Searches , social queries for CATACLYSMIC VARIABLE-STAR
Search references for CATACLYSMIC VARIABLE-STAR. Phrases containing CATACLYSMIC VARIABLE-STAR
See searches and references containing CATACLYSMIC VARIABLE-STAR!
Search references for CATACLYSMIC VARIABLE-STAR. Phrases containing CATACLYSMIC VARIABLE-STAR
See searches and references containing CATACLYSMIC VARIABLE-STAR!CATACLYSMIC VARIABLE-STAR
Stars with irregular large fluctuations in brightness
In astronomy, cataclysmic variable stars (CVs) are stars which irregularly increase in brightness by a large factor, then drop back down to a quiescent
Cataclysmic_variable_star
Cataclysmic variable star, consisting of a close binary star system
(pl. novae), or U Geminorum variable, is one of several types of cataclysmic variable star, consisting of a close binary star system in which one of the
Dwarf_nova
Highly magnetic type of cataclysmic variable binary star system
polar is a highly magnetic type of cataclysmic variable (CV) binary star system, originally known as an AM Herculis star after the prototype member AM Herculis
Polar_(star)
Type of cataclysmic variable star
star (AM CVn star) is a rare type of cataclysmic variable star named after their type star, AM Canum Venaticorum. In these hot blue binary variables,
AM_Canum_Venaticorum_star
Shock wave caused by blowing stellar wind
plasma in the Orion Nebula. Bow shocks also appear around six Cataclysmic variable star (CVs) with luminous accretion disks, which drive fast winds into
Bow_shock
Topics referred to by the same term
album Shockwave Supernova Cataclysm (film), a 1980 American film Cataclysmic variable star, which irregularly increases in brightness by a large factor,
Cataclysm
Star system in the constellation Leo
approximately 990 light-years from the Sun based on parallax. It is a cataclysmic variable star of the AM Herculis-type also known as polars. The system comprises
DP_Leonis
astronomy, a superhump is a periodic brightness variation in a cataclysmic variable star system, with a period within a few percent of the orbital period
Superhump
Type of variable star
SW Sextantis variable stars are a kind of cataclysmic variable star; they are double-star systems in which there is mass transfer from a red dwarf to a
SW_Sextantis_variable
Cataclysmic variable star in the constellation Perseus
UV Persei (UV Per) is a cataclysmic variable star of the SU Ursae Majoris subclass of dwarf novae, located in the constellation Perseus. It is catalogued
UV_Persei
Star in the constellation Andromeda
And) is an eclipsing cataclysmic variable star in the constellation Andromeda. It has been classified as a SW Sextantis variable, and its apparent visual
PX_Andromedae
Topics referred to by the same term
equal to one hundredth of a newton Classical nova, a type of cataclysmic variable star Cn (digraph), a digraph used in English for a few words of Greek
CN
Cataclysmic binary star system in the constellation Hydra
Hydrae is an eclipsing intermediate polar (DQ Herculis) -type cataclysmic variable star that also undergoes eclipses. The system varies in apparent magnitude
EX_Hydrae
Constellation in the southern celestial hemisphere
star is Alpha Pictoris, a white main-sequence star around 97 light-years away from Earth. Pictor also hosts RR Pictoris, a cataclysmic variable star system
Pictor
Star in the constellation Pictor
TW Pictoris is a 14th magnitude cataclysmic variable star system in the southern constellation of Pictor. It is located at a distance of approximately
TW_Pictoris
Variable star in the constellation Aquila
Aquilae is a cataclysmic variable star in the north of the equatorial constellation of Aquila. It is in the sub-set of nova-like (NL) variables, specifically
V1315_Aquilae
Stellar binary star system
of Hercules. It is considered a cataclysmic variable with the white dwarf pulling outer layers of hydrogen from the star onto itself. It has the shortest
ZTF_J1813+4251
X-ray source that only emits soft X-rays
the hydrogen layer to helium. Apparently the only SSXS nonmagnetic cataclysmic variable is V Sagittae: bolometric luminosity of (1–10) × 1037, a binary including
Supersoft_X-ray_source
Variable star in the constellation Sagitta
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 so far
V_Sagittae
Graph of light intensity of a celestial object or region, as a function of time
Cepheid variables, other periodic variables, and transiting extrasolar planets; or aperiodic, like the light curve of a nova, cataclysmic variable star, supernova
Light_curve
Star in the constellation Eridanus
Eridanus)[citation needed] is a variable star of the type known as polars, AM Herculis stars, or magnetic cataclysmic variable stars. Historically it has varied
EF_Eridani
Type of binary star system with a white dwarf and main-sequence star
Star) is a type of cataclysmic variable, binary star system with a white dwarf and a cool main-sequence secondary star. In most cataclysmic variables
Intermediate_polar
Observatory
for astronomical research. Farm Cove Observatory took part in cataclysmic variable star (CV) research for the Center for Backyard Astrophysics and was
Farm_Cove_Observatory
Topics referred to by the same term
(satellite), a satellite launched by NASA in 1996 Polar (star), a strongly magnetic cataclysmic variable star system POLAR III and POLAR II, a pedestrian test
Polar
Eclipsing post-common envelope binary star system in the constellation Serpens
Richard F. Green et al. found the star in the Palomar Green Survey, and determined it to be a possible cataclysmic variable star. They gave it the name PG 1550+131
NN_Serpentis
Star in the constellation of Grus
nova-like variables, which have periods of around 3 to 4 hours). It belongs to the UX Ursae Majoris subgroup of cataclysmic variable star systems, where
RZ_Gruis
Star whose brightness fluctuates, as seen from Earth
A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes systematically with time. This variation may be caused
Variable_star
Substellar object
described as the brown-dwarf desert. The PCEB might evolve into a cataclysmic variable star (CV*) with the brown dwarf as the donor. Simulations have shown
Brown_dwarf
Star in the constellation Hercules
variable star located in the constellation Hercules. This star, along with the star AN Ursae Majoris, is the prototype for a category of cataclysmic variable
AM_Herculis
Dim, low mass stars on the main sequence
red dwarfs Cataclysmic variable star – Stars with irregular large fluctuations in brightness Nemesis (hypothetical star) – Hypothetical star orbiting the
Red_dwarf
Star in the constellation Perseus
Aquilae 1918 to something resembling a typical dwarf nova-type cataclysmic variable star. The 2015 GK Per outburst peaked at magnitude 9.6, and the last
GK_Persei
Type of variable star
A slow irregular variable (ascribed the GCVS types L, LB and LC) is a variable star that exhibit no or very poorly defined periodicity in their slowly
Slow_irregular_variable
Classification in astronomy
In astronomy, the term compact object (or compact star) refers collectively to white dwarfs, neutron stars, and black holes. It could also include exotic
Compact_object
Constellation in the northern celestial hemisphere
as the secondary star is filling its Roche lobe and transferring matter to the primary. RW Ursae Minoris is a cataclysmic variable star system that flared
Ursa_Minor
Nova event seen in 1887 in the constellation Perseus
(1983). "The Periods of Cataclysmic Variable Stars". Cataclysmic Variables and Related Objects. IAU Colloq. 72: Cataclysmic Variables and Related Objects
V_Persei
Cataclysmic variable star in the constellation Dorado
BB Doradus or BB Dor is a cataclysmic variable, a pre-nova star, thus a close pair binary star system. It is composed of a red dwarf and a white dwarf
BB_Doradus
Low-mass hypervelocity star
massive white dwarf, which would have involved mass transfer in a cataclysmic variable star. The predicted ejection speed for this scenario agrees with the
CWISE_J1249+3621
Possible red cataclysmic variable star in the constellation Andromeda
M31 RV is a possible red cataclysmic variable star located in the Andromeda Galaxy (M31) that experienced an outburst in 1988, which was similar to the
M31_RV
Variable star in the constellation Draco
giant, which itself appeared to be a binary cataclysmic variable star, making the complete system a triple star. However a 2003 study by Peter Wheatley et
4_Draconis
Variable star in the constellation Ursa Major
eclipsing binary star system in the northern circumpolar constellation of Ursa Major, abbreviated DW UMa. It is a cataclysmic variable of the SX Sextanis
DW_Ursae_Majoris
System of two stars orbiting each other
potential energy, causing the gas to become hotter and emit radiation. Cataclysmic variable stars, where the compact object is a white dwarf, are examples of
Binary_star
Topics referred to by the same term
Chuvash language, a Turkic language of Russia (ISO 639-1 code CV) Cataclysmic variable star, characterized by irregular and large increases in brightness
CV
Topics referred to by the same term
USCGC Polar Star (WAGB-10), an icebreaker Polestar Xeus, a solution for monitoring cloud systems Polar (cataclysmic variable star), a type of star Order of
Polestar_(disambiguation)
Ancient Chinese term for cataclysmic variable stars
that guest stars are manifestations of cataclysmic variable stars: novae and supernovae. The term "guest star" is used in the context of ancient records
Guest_star_(astronomy)
Star in the constellation Sagittarius
V1017 Sagittarii is a cataclysmic variable star system in the constellation Sagittarius. Ida E. Woods discovered the star on Harvard College Observatory
V1017_Sagittarii
Study of how astronomical objects change with time
observations List of exoplanets detected by microlensing X-ray transient Cataclysmic variable star Stellar pulsation Schmidt, Brian (20 April 2012). "Optical Transient
Time-domain_astronomy
Large asteroid in the asteroid belt
Maunakea Observatories, but the effort came up empty. The reputed cataclysmic variable star CV Aquarii, discovered in 1934 by Emily Hughes at Harvard College
52_Europa
Variable star in the constellation Leo Minor
RZ Leonis Minoris is a cataclysmic variable star system in the northern constellation of Leo Minor. It undergoes frequent outbursts that vary in brightness
RZ_Leonis_Minoris
Constellation in the northern celestial hemisphere
Borealis is home to two remarkable variable stars. T Coronae Borealis is a cataclysmic variable star also known as the Blaze Star. Normally placid around magnitude
Corona_Borealis
Wide-field sky survey at Palomar Observatory
during its Twilight Survey. A search of ZTF's images identified cataclysmic variable star ZTF J1813+4251, a binary with a period of under 1 hour. AT2021lwx
Zwicky_Transient_Facility
Variable star in the constellation Apus
of Variable Stars as a cataclysmic variable star, it appears that it is a pulsating variable star, and has been classed as an RV Tauri variable star, type
Z_Apodis
Constellation in the northern celestial hemisphere
days. RW Trianguli is a cataclysmic variable star system composed of a white dwarf primary and an orange main sequence star of spectral type K7 V. The
Triangulum
Variable star in the constellation Andromeda
binary star system consisting of a red giant and a white dwarf. It is the prototype of a type of cataclysmic variable star known as symbiotic variable stars
Z_Andromedae
Large self-illuminated object in space
may overflow to the other star, yielding phenomena including contact binaries, common-envelope binaries, cataclysmic variables, blue stragglers, and Type
Star
Star in the constellation Camelopardalis
Z Camelopardalis (Z Cam) is a cataclysmic variable star system in the northern constellation of Camelopardalis. It has an apparent visual magnitude which
Z_Camelopardalis
Star system in the constellation Ara
ASKAP J1745−5051 (ASKAP J174508.9−505149) is a magnetic cataclysmic variable binary star in the constellation Ara with radio emission. It has been described
ASKAP_J1745−5051
Constellation in the southern celestial hemisphere
magnitude of 8.05, it is 707 ± 6 light-years distant. AH Mensae is a cataclysmic variable star system composed of a white dwarf and a red dwarf that orbit each
Mensa_(constellation)
Star in the constellation Andromeda
DX Andromedae (often abbreviated to DX And) is a cataclysmic variable star in the constellation Andromeda. It has a typical apparent visual magnitude
DX_Andromedae
Binary star in the constellation Auriga
is a binary star in the constellation Auriga, at a distance of about 1,930 light-years (590 parsecs). It is a magnetic cataclysmic variable, consisting
Paloma_(star)
Star in the constellation Ursa Minor
SS Ursae Minoris is a cataclysmic variable star system in the constellation Ursa Minor. It was discovered visually and by its X-ray emissions separately
SS_Ursae_Minoris
Slow irregular eruptive variable stars
Telescopii. Dwarf nova – Cataclysmic variable star, consisting of a close binary star system Nova – Nuclear explosion in a white dwarf star Supernova – Astrophysical
Symbiotic_nova
Star in the constellation Perseus
NSV 1436 is a cataclysmic variable star in the constellation Perseus. It is a probable U Geminorum-type dwarf nova, and outbursts have been observed in
NSV_1436
Large main-belt asteroid
mistaken for the 15th-magnitude star TU Leonis, which led to that star's classification as a U Geminorum cataclysmic variable star. Flora had come to opposition
8_Flora
Overview of the scientific field of astronomy
blue variable Gamma Cassiopeiae variable R Coronae Borealis variable Eruptive binary RS Canum Venaticorum variable Cataclysmic or explosive Cataclysmic variable
Outline_of_astronomy
Stellar explosion with a distinct red colour
merger would likely not take place at the predicted time. Binary star Cataclysmic variable star Dwarf nova Hypernova Nova Supernova Kulkarni, S. R.; Ofek, E
Luminous_red_nova
Class of astronomical objects
symbiotic binaries show brightness changes and are classified as variable stars. The star Z Andromedae is often considered the prototype of the symbiotic
Symbiotic_binary
Star in the constellation Aquarius
star, then called RXJ2107.9-0518, was both an eclipsing binary and a cataclysmic variable. The star had been flagged as a probable AM Herculis star from
HU_Aquarii
Binary star system in the constellation Fornax
well as the EXOSAT satellite that detected it. UZ Fornacis is a cataclysmic variable. The two stars, a white dwarf and red dwarf, orbit each other every
UZ_Fornacis
Cataclysmic variable star system in the constellation Andromeda
days. RX Andromedae is a cataclysmic variable system, where a white dwarf with a mass of 0.8 M☉ and an M2 main sequence star are rotating around their
RX_Andromedae
Supposed disastrous doomsday scenario
the Nibiru cataclysm often cite the winged sun symbol as actually representing Nibiru, whom they believe would appear like a "winged star". Though Lieder
Nibiru_cataclysm
Binary system consisting of a white dwarf and a main sequence star or a brown dwarf
or pre-cataclysmic variable is a binary system consisting of a white dwarf or hot subdwarf and a main-sequence star or a brown dwarf. The star or brown
Post-common-envelope_binary
Star in the constellation Mensa
a cataclysmic variable star of (SU Ursae Majoris subtype) in the constellation Mensa. A close binary, it consists of a white dwarf and low-mass star orbiting
TU_Mensae
1918 Nova in the constellation Monoceros
indicate that GI Mon is a non-magnetic cataclysmic variable star, meaning that the material lost from the donor star forms an accretion disk around the white
GI_Monocerotis
Variable star in constellation Cancer
DW Cancri (DW Cnc) is a cataclysmic variable (CV) star system located in the constellation of Cancer. It is classified as an intermediate polar (IP), a
DW_Cancri
Nova in the constellation Perseus
nova. A U Geminorum-type variable star or dwarf nova is a type of cataclysmic variable star consisting of a close binary star system in which one of the
V392_Persei
Constellation in the southern celestial hemisphere
sequence star—are thought to orbit each other roughly every 8.5 to 10 hours. It belongs to the UX Ursae Majoris subgroup of cataclysmic variable star systems
Grus_(constellation)
Nuclear explosion in a white dwarf star
considered to be cataclysmic variable stars. Classical nova eruptions are the most common type. This type is usually created in a close binary star system consisting
Nova
photographic)) David H. Levy, Observing variable stars : a guide for the beginner General Catalogue of Variable Stars Star portal Lists of astronomical objects
List_of_variable_stars
Double stars that show a significant interaction between their components
be complex and highly variable, and they are common sources of cataclysmic outbursts. A common type of interacting binary star is one in which one of
Interacting_binary_star
Binary star in the constellation Cancer
is a binary star system located in the northern constellation of Cancer and is part of the Beehive Cluster. It is a cataclysmic variable (CV) of the Z
SY_Cancri
Nova in the constellation Hercules
the northern constellation of Hercules in December 1934. This cataclysmic variable star was discovered on 13 December 1934 by J. P. M. Prentice from Stowmarket
DQ_Herculis
Triple star system in the constellation Cygnus
Wolf 1130 is a nearby pre-cataclysmic triple-star system consisting of a cold subdwarf of spectral type sdM3 (A), an ultramassive white dwarf (B) and
Wolf_1130
Astronomical observatory and planetarium in Auckland, New Zealand
Planet Center. 14 November 2016. Retrieved 29 November 2016. Cataclysmic variable star "MicroFUN 2005". Archived from the original on 2 January 2006
Stardome_Observatory
Double star in the constellation Caelum
approximately 9–20 billion years, RR Caeli will likely become a cataclysmic variable star due to the period's gradual shortening, leading to increasing
RR_Caeli
1885 supernova in the Andromeda Galaxy
unusual for Type Ia supernovae. Some astronomers observed the spectrum of the star visually (no photographic spectral observations were made in that time).
SN_1885A
Star in the constellation Pyxis
WX Pyxidis is a cataclysmic variable star system in the constellation Pyxis. Its X-ray emissions were discovered in 1984, after which a visual correlate
WX_Pyxidis
Binary star in the constellation of Draco
the same cataclysmic variable system in the northern constellation of Draco, abbreviated YY Dra and DO Dra, respectively. The DO Dra binary star system
DO_Draconis/YY_Draconis
Variable star in the constellation Vulpecula
QQ Vulpeculae is a cataclysmic variable binary star system in the northern constellation of Vulpecula, abbreviated QQ Vul. It has a brightness that fluctuates
QQ_Vulpeculae
White dwarf star in the constellation Cancer
UK, Chile and Germany. The system was initially identified as a cataclysmic variable on the basis of weak H-alpha emissions in the spectrum by the Sloan
WD_J0914+1914
American astronomer
Medal, which he received for his observational astronomy work on cataclysmic variable stars. "Keith Douglas Horne". University of St Andrews Research Portal
Keith_Horne_(astronomer)
Dwarf nova in the constellation Sculptor
78.23 minutes. BW Sculptoris is one of the closest and brightest cataclysmic variable stars with a brightness of about magnitude 16.5 and a distance of
BW_Sculptoris
University of Notre Dame campus
unusual dimming in the cataclysmic variable star system FO Aquarii, a binary star system featuring a white dwarf and main sequence star. In 2018, Garnavich
Sarah_L._Krizmanich_Telescope
Variable star in the constellation Ursa Major
SU UMa, is a close binary star in the northern circumpolar constellation of Ursa Major. It is a periodic cataclysmic variable that varies in magnitude
SU_Ursae_Majoris
Binary star in the constellation Monoceros
lines, published in 1933 by P. W. Merrill and associates. It has the variable star designation V694 Monoceros. This system has a typical apparent visual
MWC_560
Binary star system in the constellation Grus
emission of ionized helium. These properties suggested it may be a cataclysmic variable of the AM Herculis type. The binary period of 108.6 minutes lay within
CE_Gruis
Star in the constellation Pegasus
surface. This would result in a (recurrent) nova explosion—a cataclysmic variable star—and the luminosity of the white dwarf would rapidly increase by
IK_Pegasi
Galaxy in the constellation Ursa Major
that this object was actually a foreground variable star, or an outburst from a cataclysmic variable star. Cigar Galaxy "NASA/IPAC Extragalactic Database"
NGC_4013
Variable binary star system in the constellation Ursa Major
given the catalog identifier PG 0943+521, and was confirmed to be cataclysmic variable. In 1992, it was determined this is a dwarf nova that ranges in brightness
ER_Ursae_Majoris
Nova that appeared in 1956
RW Ursae Minoris (Nova Ursae Minoris 1956) is a cataclysmic variable star system that flared up as a nova in the constellation Ursa Minor in 1956. Although
RW_Ursae_Minoris
Binary star system in the constellation Telescopium
50–80 MG. The system is a source for X-ray emission. Variable stars Polar (cataclysmic variable) AM Herculis Rosen, S. R.; Mittaz, J. P. D.; Buckley,
QS_Telescopii
travel, tourism, insurance
CATACLYSMIC VARIABLE-STAR
CATACLYSMIC VARIABLE-STAR
CATACLYSMIC VARIABLE-STAR
CATACLYSMIC VARIABLE-STAR
CATACLYSMIC VARIABLE-STAR
CATACLYSMIC VARIABLE-STAR
CATACLYSMIC VARIABLE-STAR
CATACLYSMIC VARIABLE-STAR
CATACLYSMIC VARIABLE-STAR
travel, tourism, insurance