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Binary star system in the constellation Aquila
14 Sagittae is a binary star system in the equatorial constellation of Aquila. 14 Sagittae is the Flamsteed designation. It appears as a sixth magnitude
14_Sagittae
Red giant star in the constellation Sagitta
Gamma Sagittae, also named Telum, is the brightest star in northern constellation of Sagitta. A single star, it is visible to the naked eye with an apparent
Gamma_Sagittae
Index of articles associated with the same name
limitations, both designations link here. For the star Y Sagittae, a Mira variable y Sagittae, (14 Sagittae), a designation by John Flamsteed. This set index
Y_Sagittae
Star in the constellation Sagitta
an asterism consisting of ζ Sagittae, α Sagittae, β Sagittae, δ Sagittae, γ Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and ρ Aquilae. Consequently
Zeta_Sagittae
Variable star in the constellation Sagitta
WZ Sagittae (WZ Sge) is a dwarf nova cataclysmic star system in the constellation Sagitta. It consists of a white dwarf primary being orbited by a low
WZ_Sagittae
Star in the constellation Sagitta
Left Flag which consists of 11 Sagittae, γ Sagittae, α Sagittae, β Sagittae, δ Sagittae, ζ Sagittae, 13 Sagittae, 14 Sagittae and ρ Aquilae. Consequently
11_Sagittae
Star in the constellation Sagitta
consisting of Alpha Sagittae, Beta Sagittae, Delta Sagittae, Zeta Sagittae, Gamma Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and Rho Aquilae. Consequently
Alpha_Sagittae
Star in the constellation Sagitta
an asterism consisting of β Sagittae, α Sagittae, δ Sagittae, ζ Sagittae, γ Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and ρ Aquilae. Consequently
Beta_Sagittae
Constellation in the northern celestial hemisphere
Delta, Epsilon, Zeta, and Theta Sagittae are each multiple stars whose components can be seen in small telescopes. V Sagittae is a cataclysmic variable—a
Sagitta
Variable star in the constellation Sagitta
V Sagittae or V Sge is a cataclysmic variable in the constellation Sagitta. It is the only super soft X-ray source non-magnetic cataclysmic variable found
V_Sagittae
Binary star system in the constellation Sagitta
an asterism consisting of δ Sagittae, α Sagittae, β Sagittae, ζ Sagittae, γ Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and ρ Aquilae. Consequently
Delta_Sagittae
B4Ieq-K2Ib Vmax = 8.7m, Vmin = 18.1m V Sge V 20h 20m 14.69s +21° 06′ 10.44″ 9.6-13 7800 prototype V Sagittae variable, Vmax = 8.16m, Vmin = 13.9m, P = 0.514195 d
List_of_stars_in_Sagitta
Star in the constellation Sagitta
Epsilon Sagittae (ε Sagittae) is a solitary, yellow-hued star in the northern constellation of Sagitta. With an apparent visual magnitude of +5.64 to +5
Epsilon_Sagittae
Planetary nebula in the constellation of Sagitta
by Dorrit Hoffleit, and it was given the variable star designation UU Sagittae (UU Sge). In 1955, George O. Abell discovered a nebula in the same region
Abell_63
Type of star with a prominent spectral line due to absorption from ionized mercury
Internet Encyclopedia of Science, David Darling. Accessed on line August 14, 2008. Michaud, Georges (May 1970). "Diffusion Processes in Peculiar A Stars"
Mercury–manganese_star
Star in the constellation Delphinus
refers to an asterism consisting of this star, α, β, γ, δ, ζ, 11, 13, and 14 Sagittae stars of Sagitta to the west. Consequently, ρ Aquilae itself is known
Rho_Aquilae
Constellations recognized by the International Astronomical Union
Hydrus/Hydri, to avoid confusion with Hydra, abbreviated Hya; and Sge for Sagitta/Sagittae, to avoid confusion with Sgr for Sagittarius. When letters are taken from
IAU_designated_constellations
G-type main sequence star in the constellation Sagitta
15 Sagittae (15 Sge) is a star in the northern constellation Sagitta, located around 58 light years away from the Sun. It is visible to the naked eye as
15_Sagittae
Planetary nebula in the constellation Vulpecula
Summer Triangle. It is located in the sky a few degrees north of γ Sagittae, near the star 14 Vulpeculae. It is bright enough to be seen in binoculars. Messier
Dumbbell_Nebula
Millisecond pulsar in the constellation Sagitta
A visual band light curve for QX Sagittae, adapted from van Paradijs et al. (1988) The light from a nearby star of similar brightness is included, and
Black_Widow_pulsar
p. 5. Archived (PDF) from the original on 2018-07-15. Retrieved 2018-07-14. Kunitzsch, Paul; Smart, Tim (2006) [1986]. A Dictionary of Modern Star Names:
List_of_proper_names_of_stars
Eclipsing stellar binary
U Sagittae is an eclipsing binary star system in the northern constellation of Sagitta. It has been actively studied since its discovery in 1901. The maximum
U_Sagittae
Double star in the constellation Sagitta
Theta Sagittae (θ Sagittae) is a double star in the northern constellation of Sagitta. With a combined apparent visual magnitude of +6, it is near the
Theta_Sagittae
Star in the constellation Sagittarius
There are few other suspected "born-again" objects, one example being FG Sagittae. Having erupted in 1995, it is expected that Sakurai's Object's final helium
Sakurai's_Object
Ofpe/WN9 >23 WR 124 (QR Sagittae) 21,000 ± 2,000 WN8h 11.50±0.11 WR 30a 21,917+1,400 −1,090 WO4 WR 121-16 23,190 WN7o/WC 14.02 Cygnus X-3 (WR 145a/V1521
List_of_Wolf–Rayet_stars
Nuclear explosion in a white dwarf star
ones. Consequently, the interval is shorter for high-mass white dwarfs. V Sagittae is unusual in that the time of its next eruption can be predicted fairly
Nova
Species of fish
are much the same, eating the same species of pelagic crustaceans and Sagittae. Specimens of Atlantic Mackerel taken at Woods Hole ate chiefly copepods
Chub_mackerel
Constellation in the northern celestial hemisphere
classified as a slow nova, similar to DQ Herculis. Like DQ Herculis, WZ Sagittae, Nova Persei 1901 and Nova Aquilae 1918, it is a very close binary with
Auriga
F5III LSPM J0207+3331 145 ± 1 02h 07m 33.8061s +33° 31′ 29.542″ DA Theta Sagittae B 145.47 ± 0.09 Sagitta 20h 09m 56.2404s +20° 55′ 04.230″ G5V +8.769 A
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
Constellations that are no longer widely recognised
1679 Edmund Halley Rosa Rosae Rose 1536 Petrus Apianus Sagitta Australis Sagittae Australis Southern Arrow 1613 Petrus Plancius Scarabaeus Scarabaei Rhinoceros
Former_constellations
Stars with irregular large fluctuations in brightness
Louisiana State. "Binary star V Sagittae to explode as very bright nova by century's end". phys.org. Retrieved 2024-07-14. NASA (2017-12-11). "Introduction
Cataclysmic_variable_star
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
269896 HDE 269128 (R81 in LMC), LBV candidate, eclipsing binary system. HT Sagittae M33 OB21 108 MAC 1-277 V430 Scuti V452 Scuti, LBV candidate V1429 Aquilae
Hypergiant
Constellation in the northern celestial hemisphere
moving rapidly through space directly away from the galactic disc. The WZ Sagittae-type dwarf nova DY Canis Minoris (also known as VSX J074727.6+065050) flared
Canis_Minor
Gruis Star 3.47 3.41 Sigma Canis Majoris (Nganurganity) Star 3.47 Gamma Sagittae (Telum) Star 3.47 Gamma Ceti Triple star system 3.48 Eta Leonis Multiple
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Constellation in the northern hemisphere
discovered in Coma Berenices. In 1995, there was a very rare outburst of the WZ Sagittae-type dwarf nova AL Comae Berenices. A June 2003 outburst from GO Comae
Coma_Berenices
b 60 835 2019 15 Sagittae Sagitta 20h 04m 06s +17° 04′ 13″ 5.80 57.7 G1V+L4-5 B 65 14 2002 Zeta Delphini Delphinus 20h 35m 19s +14° 40′ 27″ 4.65 220
List_of_brown_dwarfs
5624±0.2525 B G8III-IV Iota Trianguli B 260 ± 10 Triangulum F5V 6.83 Zeta Sagittae 260 ± 10 Sagitta A3 Vnn +5.00 13 Comae Berenices 260 ± 20 Coma Berenices
List of star systems within 250–300 light-years
List_of_star_systems_within_250–300_light-years
M3-M4.5 (M2.5-M5Iae) 1420±120 17±8 270000±40000 6.5-9.6 HD 183143 (HT Sagittae) 4990±550 B6-8 Ia-0 109±15 24.2±1.4 288000+83000 −65000 6.71-6.95 HD 168625
List_of_nearest_hypergiants
Dwarf nova star in the constellation Andromeda
Majoris variable. The variability of LL Andromedae is similar to the WZ Sagittae type of dwarf novae. Those have a long outbursts cycle (they were observed
LL_Andromedae
Smith. Archived from the original on August 14, 2017. Retrieved August 15, 2017. Mathewson, Samantha (November 14, 2016). "'Supermoon' Science: NASA Explains
List of future astronomical events
List_of_future_astronomical_events
Star that has a supergiant luminosity class, with a spectral type of F or G
of the Field RV Tauri Variables: EP Lyrae, DY Orionis, AR Puppis, and R Sagittae". The Astrophysical Journal. 479 (1): 427–440. Bibcode:1997ApJ...479..427G
Yellow_supergiant
DAZ HD 23753 420 ± 10 B9 Vn 5.44 Part of Pleiades Cluster (M45). Beta Sagittae (Shakh) 420 ± 10 Sagitta G8 IIIa CN 0.5 4.38 HD 136138 (HR 5692) A 420
List of star systems within 400–450 light-years
List_of_star_systems_within_400–450_light-years
Minor. Named after Masaaki Huruhata [ja]. Huruhata's Variable is the WZ Sagittae type dwarf nova EG Cancri. Huth's "moving star" of 1801-2, discovered and
Stars_named_after_people
American astronomer (1927–2021)
doi:10.1086/182401. Bond, H. E.; Liller, W.; Mannery, E. J. (1978). "UU Sagittae - Eclipsing nucleus of the planetary nebula Abell 63". The Astrophysical
William_Liller
the subclass UGWZ – (celestial object) UG WZ Sagittae, a subclass of UG-type stars named after WZ Sagittae, the archetype for the subclass UGZ – (celestial
List_of_astronomy_acronyms
Genus of fishes
Bellstedt, 2019 Nothobranchius ruudwildekampi Costa, 2009 Nothobranchius sagittae Wildekamp, Watters & Shidlovskiy, 2014 Nothobranchius sainthousei Nagy
Nothobranchius
represent the volume that the work is part of. Ad Dominum cum tribularer. Sagittae potentis (5) Adoramus te, Christe (5) Ad te levavi oculos meos. Miserere
List of compositions by Giovanni Pierluigi da Palestrina
List_of_compositions_by_Giovanni_Pierluigi_da_Palestrina
Genus of fishes
P. Gosse, 1966) Amphilophus margaritifer (Günther, 1862) Amphilophus sagittae Stauffer & McKaye, 2002 Amphilophus supercilius Geiger, McCrary & Stauffer
Amphilophus
Type of variable star
Bibcode:1953ZA.....32..125K. Watson, Christopher (4 January 2010). "S Sagittae". AAVSO Website. American Association of Variable Star Observers. Retrieved
Classical_Cepheid_variable
Paul; Parsons, Steven G.; Riddle, Reed L.; Rusholme, Ben; Sahman, Dave I. (14 August 2023). "A rotating white dwarf shows different compositions on its
List_of_smallest_known_stars
Star in the constellation Crux
are now discounted include WR 46 being a Super soft X-ray source or a V Sagittae star, The radial velocity changes of the spectral lines originating most
WR_46
Class of luminous variable star
the distinctive variations in brightness of R Scuti from 1840 to 1850. R Sagittae was noted to be variable in 1859, but it was not until the discovery of
RV_Tauri_variable
Has one exoplanet (b / Baiduri) HD 181327 155.8 ± 0.2 F6V 7.04±0.01 Eta Sagittae 155.9 ± 0.9 Sagitta K2 III +5.09 Beta Apodis 156 ± 1 Apus K0 III +4.24
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
"Long-Period Objects in the Extrasolar Planetary Systems 47 Ursae Majoris and 14 Herculis". The Astrophysical Journal. 654 (1): 625–632. arXiv:astro-ph/0609117
List of star systems within 55–60 light-years
List_of_star_systems_within_55–60_light-years
Star in the constellation Perseus
the period is less than two hours. That would mean that it could be a WZ Sagittae type of dwarf nova, but the lack of superhumps and relatively small outburst
NSV_1436
Star in the constellation Perseus
R. E. (November 1986), "The asynchronously rotating Algol binaries U Sagittae and RY Persei", Astronomical Journal, 92: 1168–1177, Bibcode:1986AJ...
RY_Persei
Polish astronomer
Geminorum. In 1964, Krzemiński and Robert Kraft discovered that the star WZ Sagittae (WZ Sge) is a cataclysmic new dwarf of circulation one hour and 22 minutes
Wojciech_Krzemiński
that the wedding of Jezebel and Ahab was the likely occasion, reading verse 14 as originally referring not to a "King's daughter who is within" but a "daughter
Psalm_45
Binary star system in the constellation Serpens
Bright Double-lined Spectroscopic Binaries. VIII. HR 1528, HR 6993, 2 Sagittae, and 18 Vulpeculae". The Astronomical Journal. 146 (5). 129. Bibcode:2013AJ
HD_171978
1283 battle part of the War of the Sicilian Vespers
twenty-four oars A light galley with around one hundred oars Probably three sagittae, or "arrows" which were small scouting vessels of up to sixteen oars The
Battle_of_Malta_(1283)
by Edward Emerson Barnard. Harlow Shapley finds that the spectrum of S Sagittae and other Cepheid variables varies with brightness, recording it as spectral
1916_in_science
1976 Nova seen in the constellation Vulpecula
265..314M. doi:10.1038/265314a0. S2CID 4174860. Hughes DW (1977). "Nova sagittae 1977 and vulpeculae 1976". Nature. 265 (5594): 500. Bibcode:1977Natur.265
NQ_Vulpeculae
Binary star in the constellation Auriga
Bright Double-lined Spectroscopic Binaries. VIII. HR 1528, HR 6993, 2 Sagittae, and 18 Vulpeculae" (PDF), The Astronomical Journal, 146 (5): 20, Bibcode:2013AJ
HD_30453
Dwarf nova in the constellation Andromeda
star is only 0.07 M☉. This low mass makes V455 Andromedae similar to WZ Sagittae dwarf novae, which are expected to have a long period between outbursts
V455_Andromedae
Eclipsing binary star in the constellation Taurus
"Determination of the Elements of Eclipsing Variables RW Tauri and U Sagittae by an Analysis of the Light Changes in the Frequency Domain", Astrophysics
RW_Tauri
14 SAGITTAE
14 SAGITTAE
Male
English
English and French form of Latin Paulus, PAUL means "small." In the bible, this is the name of the author of the 14 epistles of the New Testament.
Boy/Male
Irish
Is the Irish form of Old English ead “â€richâ€â€ + mund “â€guardianâ€â€, and implies “â€guardian of the riches.â€â€ In more recent times the name has been given to honor Eamon De Valera who was President of Ireland for 14 years, the maximum allowed, from 1959 to 1973.
Boy/Male
Irish
Is the Irish form of Old English ead “â€richâ€â€ + mund “â€guardianâ€â€, and implies “â€guardian of the riches.â€â€ In more recent times the name has been given to honor Eamon De Valera who was President of Ireland for 14 years, the maximum allowed, from 1959 to 1973.
Surname or Lastname
English and Scottish
English and Scottish : from a medieval personal name, Latin Valentinus, a derivative of Valens (see Valente), which was never common in England, but is occasionally found from the end of the 12th century, probably as the result of French influence. The name was borne by a 3rd-century saint and martyr, whose chief claim to fame is that his feast falls on February 14, the date of a traditional celebration of spring going back to the Roman fertility festival of Juno Februata. A 5th-century missionary bishop of Rhaetia of this name was venerated especially in southern Germany, being invoked as a patron against gout and epilepsy.
Male
Greek
(ΠαÏλος) Greek form of Latin Paulus, PAULOS means "small." In the bible, this is the name of the author of the 14 epistles of the New Testament.
Boy/Male
Irish
Is the Irish form of Old English ead “â€richâ€â€ + mund “â€guardianâ€â€, and implies “â€guardian of the riches.â€â€ In more recent times the name has been given to honor Eamon De Valera who was President of Ireland for 14 years, the maximum allowed, from 1959 to 1973.
14 SAGITTAE
14 SAGITTAE
14 SAGITTAE
14 SAGITTAE
14 SAGITTAE
14 SAGITTAE
14 SAGITTAE