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Variable stars which exhibit non-radial pulsations
Alpha Cygni variables are variable stars which exhibit non-radial pulsations, meaning that some portions of the stellar surface are contracting at the
Alpha_Cygni_variable
Blue supergiant star in the constellation Cygnus
acute angles. The spectrum of Alpha Cygni has been observed by astronomers since at least 1888, and by 1910 the variable radial velocity had become apparent
Deneb
Type of star that is luminous, blue, and variable in brightness
also known as S Doradus variables after S Doradus, one of the brightest stars of the Large Magellanic Cloud. The LBV stars P Cygni and η Carinae have been
Luminous_blue_variable
Star in the constellation Cygnus
supergiant variable, but subsequent studies have treated it as an Alpha Cygni variable. It shows pulsations with multiple periods from a few hours to 22
55_Cygni
Variable star in the constellation Cygnus
P Cygni (34 Cygni) is a variable star in the constellation Cygnus. The designation "P" was originally assigned by Johann Bayer in Uranometria as a nova
P_Cygni
Brightest star in the constellation Orion
apparent magnitude ranging from 0.05 to 0.18. It is classified as an Alpha Cygni variable due to the amplitude and periodicity of its brightness variation
Rigel
Yellow hypergiant in the Large Magellanic Cloud
referred to as G266 and R92, is a rare yellow hypergiant (YHG) and an Alpha Cygni variable. It is one of the brightest stars in the Large Magellanic Cloud (LMC)
HD_271182
Star whose brightness fluctuates, as seen from Earth
of variable is PV Telescopii, which undergoes small but complex luminosity variations and radial velocity fluctuations. Alpha Cygni (α Cyg) variables are
Variable_star
Star in the constellation Cygnus
consisting of Gamma Cygni, Delta Cygni, 30 Cygni, Alpha Cygni, Nu Cygni, Tau Cygni, Upsilon Cygni, Zeta Cygni and Epsilon Cygni. Consequently, the Chinese
Gamma_Cygni
Star in the constellation of Puppis
variations had been thought to be the due to the pulsations of an α Cygni variable, but are too predictable and regular. The eclipse-like light curve is
Zeta_Puppis
Blue supergiant star in the constellation Canis Major
in the final stages of its life. The star is classified as an Alpha Cygni-type variable star and its brightness varies from magnitude +2.38 to +2.48 over
Eta_Canis_Majoris
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
A. M.; Sterken, C. (1999). "Light variations of massive stars (alpha Cygni variables). XVII. The LMC supergiants R 74 (LBV), R 78, HD 34664 = S 22 (B[e]/LBV)
Hypergiant
Star in the constellation Orion, in the center of the Orion's Belt
December 15. It is slightly variable from magnitude 1.64 to 1.74, with no clear period, and it is classified as an α Cygni variable. Its spectrum also varies
Alnilam
Binary star system in the Cygnus constellation
61 Cygni /ˈsɪɡni/ is a binary star system in the northern constellation Cygnus, consisting of a pair of K-type dwarf stars that orbit each other in a
61_Cygni
Star in the constellation Cygnus
NML Cygni or V1489 Cygni (abbreviated to NML Cyg or V1489 Cyg) is a red hypergiant or red supergiant (RHG or RSG) in the constellation Cygnus. It is one
NML_Cygni
Third-magnitude star in the constellation Cygnus
Delta Cygni, Gamma Cygni, 30 Cygni, Alpha Cygni (Deneb) and Nu, Tau, Upsilon, Zeta and Epsilon Cygni. Consequently, the Chinese name for Delta Cygni itself
Delta_Cygni
Star in the constellation Norma
visual magnitude between 4.87 and 4.98, and is suspected of being an Alpha Cygni variable, which are named after Deneb. It is in the same direction and at
Mu_Normae
Star in the constellation Carina
Carinae (V533 Car, y Car, y Carinae) is a A-type supergiant and a Alpha Cygni variable star with a mean apparent magnitude of about +4.6 in the constellation
V533_Carinae
Star in the constellation Sagitta
HD 183143 was formally announced as a variable star, probably of the α Cygni type, in 1979 and given the variable star designation HT Sagittae. HD 183143
HD_183143
Constellation in the northern celestial hemisphere
Retrieved 3 March 2015. BSJ (4 January 2010). "Alpha Cygni". AAVSO Website. American Association of Variable Star Observers. Retrieved 22 December 2013.
Cygnus_(constellation)
Star in Large Magellanic Cloud
was classified as a possible S Doradus variable. A 1998 paper considers it an active LBV, an Alpha Cygni variable, and a 2018 census of LBVs considers it
HD_37836
Constellation in the southern celestial hemisphere
and diameter around 80 times that of the Sun. Classified as an Alpha Cygni type variable star, Aludra varies in brightness from magnitude 2.38 to 2.48
Canis_Major
Multiple star system in the constellation Sagittarius
96). In addition, it shows more irregular variations typical of an Alpha Cygni variable, irregularly pulsating hot supergiant stars. Mu Sagittarii A appears
Mu_Sagittarii
Star in the constellation of Cygnus
lying in the sky at the centre of the triangle formed by Deneb, γ Cygni and δ Cygni. WR 140 is thought to be a prototypical example of cosmic dust production
WR_140
Star system in the Centaurus constellation
released his own accurately determined parallax for 61 Cygni in 1838. For this reason, Alpha Centauri is sometimes considered as the second star to have
Alpha_Centauri
Star in the constellation Orion
within Orion, admitting the higher published mean brightness of much more variable stars ranked above it, 35th.[citation needed] Chi1 Orionis is an unrelated
Chi2_Orionis
Variable star in the constellation Centaurus
Centauri is a white A-type blue supergiant. It is classified as an Alpha Cygni type variable star and its brightness varies from magnitude +5.12 to +5.22 with
Omicron2_Centauri
Star in the constellation Cassiopeia
around 9,600 light years. HD 223960 is tentatively classified as an α Cygni variable; its brightness changes erratically by less than a tenth of a magnitude
HD_223960
Star in the constellation Cygnus
consisting of Epsilon Cygni, Gamma Cygni, Delta Cygni, 30 Cygni, Alpha Cygni, Nu Cygni, Tau Cygni, Upsilon Cygni and Zeta Cygni. Consequently, the Chinese
Epsilon_Cygni
Star in the constellation Cassiopeia
slightly hotter than a standard B1 star. It is classified as an Alpha Cygni type variable star and its brightness varies by a few hundredths of a magnitude
Kappa_Cassiopeiae
Overview of the scientific field of astronomy
Other RV Tauri variable Alpha Cygni variable Pulsating white dwarf Eruptive Pre-main sequence star Herbig Ae/Be Orion variable FU Orionis star Main Sequence
Outline_of_astronomy
Supergiant star in the constellation Vela
classification F8Ib. b Velorum has been classified as a suspected α Cygni variable star which varies by only 0.06 magnitude. There are possible periods
HD_74180
Type of star that is massive and luminous
as Alpha Cygni variables, semiregular variables, and irregular variables show some degree of photometric variability, certain types of variables amongst
Supergiant
Hot, luminous star with a spectral type of A9 or earlier
Wolf Rayet star.[citation needed] Many blue supergiant stars are Alpha Cygni variables. While the stellar wind from a red supergiant is dense and slow
Blue_supergiant
"Identification of a Constellation from a Position". Retrieved 2006-12-26. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Sagitta
Asterism
Beta and Gamma Cygni formed the pole of the Christian Cross, while Delta and Epsilon formed the cross beam. The variable star P Cygni was then considered
Northern_Cross_(asterism)
Variable star in the constellation Carina
Cyril; Meynet, Georges (2013). "Evolution of blue supergiants and α Cygni variables: Puzzling CNO surface abundances". Monthly Notices of the Royal Astronomical
HD_96919
Blue supergiant star in the constellation Perseus
fusing heavier elements. It is an Alpha Cygni variable (designated V474 Persei), a type of non-radial pulsating variable. It ranges in magnitude from 5.15
9_Persei
Star in the constellation Crux
known variable class B stars found that HR 4887 is variable by about a tenth of a magnitude. It is thought likely to be an α Cygni-type variable. Roman
HR_4887
Star in the constellation Scorpius
Tijdhof, W. (August 1989). "Light variations of massive stars (alpha Cygni variables). IX". Astronomy and Astrophysics Supplement Series. 79: 263–282
HD_151804
Binary star in the constellation Camelopardalis
be a variable star when the Hipparcos data was analyzed. It was given its variable star designation in 1999. It is classified as an Alpha Cygni type variable
CS_Camelopardalis
Star in the constellation Cepheus
star. 9 Cephei was given the name V337 Cephei and classified as an α Cygni variable in 1979. It varies irregularly between magnitude 4.69 and 4.78. A study
9_Cephei
Star in the constellation Cepheus
from ν Cephei, and abbreviated Nu Cep or ν Cep. This is a pulsating α Cygni variable star that ranges in apparent visual magnitude from 4.25 to 4.35. This
Nu_Cephei
Star in the constellation Gemini
pulsating variable and a close double star, with a mean combined apparent visual magnitude of about 5.7. 3 Geminorum was found to be an α Cygni variable in 1998
3_Geminorum
Star in the constellation Dorado
M.; Zegelaar, I. (1998). "Hipparcos photometry of 24 variable massive stars (α Cygni variables)". Astronomy and Astrophysics Supplement Series. 128:
HD_33579
Variable star in the constellation Leo
930 light-years (900 parsecs) from the Earth. Rho Leonis is an Alpha Cygni-type variable star, showing 0.032 magnitude brightness variations with a period
Rho_Leonis
Region of an astronomical diagram
helium. Most high luminosity supergiants are somewhat variable, including the Alpha Cygni variables. In the specific region of more luminous stars above
Instability_strip
Star in the constellation Norma
M.; Zegelaar, I. (1998). "Hipparcos photometry of 24 variable massive stars (α Cygni variables)". Astronomy and Astrophysics Supplement Series. 128:
QU_Normae
Constellation in the southern celestial hemisphere
suspected of being an Alpha Cygni variable, with a magnitude range of 4.87–4.98. QU Normae is another hot blue-white star that is a variable, ranging from magnitude
Norma_(constellation)
Binary star in the constellation Scorpius
Scorpius. It has the Bayer designation α Scorpii, which is Latinised to Alpha Scorpii. Often referred to as "the heart of the scorpion", Antares is flanked
Antares
Star in the constellation Cassiopeia
000 times as luminous. The star is slightly and erratically variable, an Alpha Cygni variable. Not all sources consider 6 Cas to be a hypergiant. It is
6_Cassiopeiae
Variable star in constellation Canis Major
blue-white hue of a B-type star. This star is classified as an Alpha Cygni-type variable star that undergoes periodic non-radial pulsations, which cause
Omicron2_Canis_Majoris
Star in the constellation Dorado
to hundreds of days. The faster variations are characteristic of α Cygni variables, irregular pulsating supergiants. The slower variations are accompanied
HD_37974
Northern pole-star; brightest star in Ursa Minor
constellation of Ursa Minor. It is designated α Ursae Minoris (Latinized to Alpha Ursae Minoris) and is commonly called the North Star. With an apparent magnitude
Polaris
Type of variable star
type or luminosity is unclear. The K5 star CO Cygni is given as a representative example. Irregular variable supergiants of late spectral types having amplitudes
Slow_irregular_variable
Star in the constellation Crux
satellite. The variability type is unclear but it is assumed to be an α Cygni variable. DS Crucis is an A1 bright supergiant (luminosity class Ia), although
DS_Crucis
Star in the constellation Crux
Catalogue of Variable Stars, but the International Variable Star Index classifies it as an α Cygni variable with a visual magnitude range of 6.82 - 7.01. van
BU_Crucis
Star in the constellation Sagittarius
to be a variable star in 1996, when the Hipparcos data was analysed. A white supergiant of spectral type A2/A3Iab, it is an Alpha Cygni variable that varies
V4381_Sagittarii
Star in the constellation Sagittarius
(V4030 Sagittarii) is a blue hypergiant star and candidate luminous blue variable located in the constellation of Sagittarius easy to see with amateur telescopes
HD_168625
Topics referred to by the same term
designation for the 15th variable star named in a constellation: RW Cephei, an orange hypergiant located in the constellation Cepheus RW Cygni, a red supergiant
RW
Variable star in the constellation Scorpius
be a variable star in 1996, when the Hipparcos data was analysed. It was given its variable star designation in 1999. It is an α Cygni variable; a supergiant
V1073_Scorpii
Nebula near the star Sadr
1318 (also known as Gamma Cygni Nebula) is the diffuse emission nebula and a H II region surrounding the star Sadr (γ Cygni) at the center of Cygnus's
IC_1318
Star in the constellation Camelopardalis
HD 21389 is a supergiant variable star in reflection nebula VdB 15, in the constellation Camelopardalis. It has the variable star designation CE Camelopardalis
HD_21389
Star in the constellation Crux
of 2 days 21 hours It was classified as an α Cygni variable. Shortly afterwards it received its variable star designation of DL Crucis. A later detailed
DL_Crucis
Star in the constellation Carina
automated classification from Hipparos photometry suggested it is an α Cygni variable. The observed brightness varies from magnitude +4.63 to +4.72. V399
V399_Carinae
Blue supergiant star in the constellation Perseus
constellation Perseus. Its apparent magnitude is 6.26 although it is slightly variable. 10 Persei is located around 3,333 parsecs (10,870 ly) distant in the Perseus
10_Persei
Variable star in the constellation Cygnus
X Cygni is a variable star in the northern constellation of Cygnus, abbreviated X Cyg. This is a Delta Cephei variable that ranges in brightness from an
X_Cygni
Pattern of stars recognized on Earth's night sky
simple geometric shapes. The Summer Triangle of Deneb, Altair, and Vega – α Cygni, α Aquilae, and α Lyrae – is prominent in the northern hemisphere summer
Asterism_(astronomy)
Constellation in the southern celestial hemisphere
Groombridge 1830 and 61 Cygni, and the ninth-highest overall. This will move the star into Tucana around 2640. It figures directly between Alpha and Beta. Indus
Indus_(constellation)
Visible star that is nearly aligned with Earth's axis of rotation
close enough to be taken as marking the pole, while third-magnitude Delta Cygni will be a more helpful pole star, at a distance of 3° from celestial north
Pole_star
chemically peculiar variable star MACS J1149 Lensed Star 1 (or Icarus) — second most distant star, 9 billion light years away. P Cygni — suddenly brightened
Lists_of_stars
FK Comae Berenices variable in the constellation Cygnus
V1794 Cygni is a single variable star in the northern constellation Cygnus. It has the identifier HD 199178 from the Henry Draper Catalogue; V1794 Cygni is
V1794_Cygni
Red supergiant star in the constellation Orion
171W. Davis, Kate (December 2000). "Variable star of the month: Alpha Orionis". American Association of Variable Star Observers (AAVSO). Retrieved 10
Betelgeuse
Star in the constellation Vela
stellar classification of B5 Ia. It is suspected to be an Alpha Cygni-type pulsating variable and ranges in brightness from 4.97 down to 5.04 magnitude
GX_Velorum
Star naming system
designations, but some have survived to refer to astronomical objects: P Cygni for example is still used as a designation for Nova Cyg 1600. Tycho's Star
Bayer_designation
Brightest star in the constellation Lyra
has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close to the Solar System
Vega
Stars with a supergiant luminosity class with a spectral type of K or M
DFK 1 Mu Cephei VV Cephei A NML Cygni S Persei UY Scuti VY Canis Majoris Westerlund 1 W26 WOH G64 A KY Cygni BI Cygni VX Sagittarii A survey expected
Red_supergiant
Constellation in the northern celestial hemisphere
constellation is Vega (Alpha Lyrae), a main-sequence star of spectral type A0Va. Only 7.7 parsecs distant, Vega is a Delta Scuti variable, varying between magnitudes
Lyra
Star in the constellation Sagittarius
; Zijderveld, M. J. (1992). "Light variations of massive stars (Alpha Cygni variables). XIII - the B-type hypergiants R81 (LBV), HD 80077 (LBV?), HD 168607
HD_168607
Class of young variable stars
1−210524b around a K-type star PDS 70b around a K-type star Orion variable EX Lupi P Cygni profile Appenzeller, I; Mundt, R (1989). "T Tauri stars". The Astronomy
T_Tauri_star
apparent magnitude of −4.05. Some stars, like Betelgeuse and Antares, are variable stars, changing their magnitude over days, months or years. In the table
List_of_brightest_stars
Continuous band of stars that appears on plots of stellar color versus brightness
known as the instability strip, is occupied by pulsating variable stars known as Cepheid variables. These stars vary in magnitude at regular intervals, giving
Main_sequence
Star in the constellation Canis Major
Cephei, S Persei, VX Sagittarii, and NML Cygni. Such stars were also referred to as "S Per et al.". The H-alpha (Hα) line is not visible yet and there are
VY_Canis_Majoris
Stellar classification
unchanged over the years, are: Sigma Draconis (K0 V) Epsilon Eridani (K2 V) 61 Cygni A (K5 V) Other primary MK standard stars include: 70 Ophiuchi A (K0 V),
K-type_main-sequence_star
Star in the constellation Cygnus
magnitudes. ξ Cygni is in the Kepler spacecraft's field of view but no planets have been detected. H-alpha RGB amateur image of ξ Cygni, center star,
Xi_Cygni
Constellation in the northern celestial hemisphere
calcium and hydrogen. Its spectral type is G5V:e. SS Aurigae is an SS Cygni-type variable star, classified as an explosive dwarf. Discovered by Emil Silbernagel
Auriga
Star in the constellation Cygnus
Flying Serpent, refers to an asterism consisting of Pi1 Cygni, Alpha Lacertae, 4 Lacertae, Pi2 Cygni, HD 206267, Epsilon Cephei, Beta Lacertae, Sigma Cassiopeiae
Pi1_Cygni
Star in the constellation Carina
By 1970, HR Carinae and the similar variable AG Carinae were recognised as being related to the P Cygni variables, unstable hot supergiants. The group
HR_Carinae
Star in the constellation Centaurus
Van Genderen, A. M. (1992). "Light variations of massive stars (Alpha Cygni variables). XII - the photometric history of the G8Ia(+) hypergiant V766 CEN
HR_5171
Systematic designations to unambiguously identify astronomical objects
star lies. Such designations mark them as variable stars. Examples include R Cygni, RR Lyrae, and V1331 Cygni. The International Astronomical Union delegates
Astronomical naming conventions
Astronomical_naming_conventions
Mysterious nearly periodic radial velocity variations in the eccentric binary ε Cygni", Astronomy & Astrophysics, 647: A160, arXiv:2102.01999, Bibcode:2021A&A
List_of_nearest_giant_stars
Tabulated list of astronomical objects
lists stars using numbers combined with constellation, for example 61 Cygni, and ordered by right ascension. The Messier catalogue: the Messier objects
Astronomical_catalogue
System of two stars orbiting each other
binaries include 61 Cygni (a binary in the constellation Cygnus, composed of two K class (orange) main-sequence stars, 61 Cygni A and 61 Cygni B, which is known
Binary_star
Process by which stars are named
Such designations mark them as variable stars. Examples include R Cygni, RR Lyrae, and GN Andromedae. (Many variable stars also have designations in
Stellar designations and names
Stellar_designations_and_names
Type of cool giant star
slow irregular variable in a symbiotic binary system with a hotter companion which may also be variable. The Mira variable Chi Cygni is an intrinsic
S-type_star
Type of star, larger and brighter than the Sun
M-type giant. Mira (ο Ceti), an M-type giant and prototype Mira variable. Chi Cygni, a S-type giant. TX Piscium, a C-type giant (carbon star). Giant
Giant_star
Star in the constellation Monoceros
(1990). "Photometry of HD 50064 - A Be supergiant star with a P Cygni profile at H-alpha". Publications of the Astronomical Society of the Pacific. 102:
HD_50064
E. N. (2009-01-01). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+, 2007-2017)". VizieR Online Data Catalog: B/gcvs. Bibcode:2009yCat
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Star in the constellation Canis Minor
designation α Canis Minoris, which is Latinized to Alpha Canis Minoris, and abbreviated α CMi or Alpha CMi, respectively. As determined by the European
Procyon
Stellar explosions that appear to be supernovae
examples of supernova impostors include the Great Eruption of Eta Carinae, P Cygni, SN 1961V, SN 1954J, SN 1997bs, SN 2008S, and SN 2010dn where detections
Supernova_impostor
ALPHA CYGNI-VARIABLE
ALPHA CYGNI-VARIABLE
Girl/Female
Indian
Little
Boy/Male
Tamil
First letter of the greek alphabet
Girl/Female
English American
Healer.
Girl/Female
Indian
Loving
Girl/Female
Biblical
According to variable songs or tunes.
Girl/Female
Gujarati, Hindu, Indian, Jain, Kannada, Malayalam, Marathi, Oriya, Sanskrit, Tamil, Telugu
Little; Collection of Many Small Things
Girl/Female
Greek American
Firstbom.' The first letter of the Greek alphabet.
Girl/Female
Tamil
Little
Boy/Male
Anglo, Australian, British, English, French, Swedish
Variable; Brave with the Spear; Spear Rule
Biblical
according to variable songs or tunes,
Male
African
(ox); the first letter of the Greek alphabet.
Boy/Male
Anglo, British, English
Variable
Girl/Female
American, British, English, Greek
Healer; With Healing Power
Boy/Male
African, Australian, Chinese, French, Latin, Swedish
First Letter of the Greek Alphabet; Leader
Surname or Lastname
English
English : from a medieval male personal name (from Latin Hilarius, a derivative of hilaris ‘cheerful’, ‘glad’, from Greek hilaros ‘propitious’, ‘joyful’). The Latin name was chosen by many early Christians to express their joy and hope of salvation, and was borne by several saints, including a 4th-century bishop of Poitiers noted for his vigorous resistance to the Arian heresy, and a 5th-century bishop of Arles. Largely due to veneration of the first of these, the name became popular in France in the forms Hilari and Hilaire, and was brought to England by the Norman conquerors.English : from the much rarer female personal name Eulalie (from Latin Eulalia, from Greek eulalos ‘eloquent’, literally well-speaking, chosen by early Christians as a reference to the gift of tongues), likewise introduced into England by the Normans. A St. Eulalia was crucified at Barcelona in the reign of the Emperor Diocletian and became the patron of that city. In England the name underwent dissimilation of the sequence -l-l- to -l-r- and the unfamiliar initial vowel was also mutilated, so that eventually the name was considered as no more than a feminine form of Hilary (of which the initial aspirate was in any case variable).
Boy/Male
Hindu
First letter of the greek alphabet
Girl/Female
Arabic
Respectable
Surname or Lastname
English (of Norman origin)
English (of Norman origin) : habitational name from Saint-Hilaire-du-Harcouët in La Manche, which gets its name from the dedication of its church to St. Hilary, or alternatively from either of the places, in La Manche and Somme, called Saint-Lô. Both of the latter are named from a 6th-century St. Lauto, bishop of Coutances; his name is of variable form in the sources and uncertain etymology.North German : habitational name for someone from Sandel.Jewish (eastern Ashkenazic) : occupational name for a cobbler or shoemaker, Yiddish sandler (from Hebrew sandelar, from Late Latin sandalarius, an agent derivative of sandalium ‘shoe’).
Surname or Lastname
English
English : topographic name for someone living on (and farming) a hide of land, Old English hī(gi)d. This was a variable measure of land, differing from place to place and time to time, and seems from the etymology to have been originally fixed as the amount necessary to support one (extended) family (Old English hīgan, hīwan ‘household’). In some cases the surname is habitational, from any of the many minor places named with this word, as for example Hyde in Greater Manchester, Bedfordshire, and Hampshire.English : variant of Ide, with inorganic initial H-. Compare Herrick.Jewish (American) : Americanized spelling of Haid.
ALPHA CYGNI-VARIABLE
ALPHA CYGNI-VARIABLE
Boy/Male
Tamil
Husband, Adored, Precious, Pleasant, Spring, Beloved by the Moon, The Moon pleasant
Boy/Male
Irish
Surname.
Girl/Female
Tamil
Sacred plant, A sacred plant (Basil)
Girl/Female
Sikh
Metrical composition
Girl/Female
Indian
Experienced
Girl/Female
Indian
Very Intelligent; Sreshta
Girl/Female
Hindu, Indian, Marathi
Auspicious
Boy/Male
Indian, Sanskrit
Lord of Kings
Girl/Female
Indian
Sweet and Beautiful
Girl/Female
Indian
Joy, Happiness, New beginning
ALPHA CYGNI-VARIABLE
ALPHA CYGNI-VARIABLE
ALPHA CYGNI-VARIABLE
ALPHA CYGNI-VARIABLE
ALPHA CYGNI-VARIABLE
n.
The quality or state of being variable; variability.
n.
Alt. of Alpia
n.
The first letter in the Greek alphabet, answering to A, and hence used to denote the beginning.
n.
The seed of canary grass (Phalaris Canariensis), used for feeding cage birds.
a.
Changeable; uncertain; inconstant; variable.
n.
That which is variable; that which varies, or is subject to change.
a.
Varying in from, character, or the like; variable; different; diverse.
n.
A shifting wind, or one that varies in force.
a.
Having the capacity of varying or changing; capable of alternation in any manner; changeable; as, variable winds or seasons; a variable quantity.
n.
A northern constellation, the Harp, containing a white star of the first magnitude, called Alpha Lyrae, or Vega.
adv.
In a variable manner.
a.
Liable to be turned in opinion; changeable; variable; unsteady; inconstant; as versatile disposition.
a.
Liable to vary; too susceptible of change; mutable; fickle; unsteady; inconstant; as, the affections of men are variable; passions are variable.
n.
The last letter of the Greek alphabet. See Alpha.
n.
A five-pointed star, resembling five alphas joined at their bases; -- used as a symbol.
n.
A quantity which may increase or decrease; a quantity which admits of an infinite number of values in the same expression; a variable quantity; as, in the equation x2 - y2 = R2, x and y are variables.
n.
The quality or state of being variable; variableness.
n.
Those parts of the sea where a steady wind is not expected, especially the parts between the trade-wind belts.
a.
Implying privation or negation; giving a negative force to a word; as, alpha privative; privative particles; -- applied to such prefixes and suffixes as a- (Gr. /), un-, non-, -less.