AM Canum Venaticorum (AM CVn) is a hydrogen-deficient cataclysmic variable binary star in the constellation of Canes Venatici. It is the type star of its class of variables, the AM Canum Venaticorum stars. The system consists of a white dwarf gaining matter via an accretion disk from a semi-degenerate or white dwarf companion.
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and 28 Related for: AM Canum Venaticorum information
AMCanumVenaticorum (AM CVn) is a hydrogen-deficient cataclysmic variable binary star in the constellation of Canes Venatici. It is the type star of its...
J0926+3624, is a star system in the constellation Leo Minor. It is an AMCanumVenaticorum-type variable star, a type of binary systems with ultra-short periods...
star and is deep red in color, with a spectral type of C54J(N3). AMCanumVenaticorum, a very blue star of magnitude 14, is the prototype of a special...
20 CanumVenaticorum is a single variable star in the northern constellation of Canes Venatici, located 238 light years from the Sun. This object has...
Binary star Orbital period. AMCanumVenaticorum 17.146 minutes Beta Lyrae AB 12.9075 days Alpha Centauri AB 79.91 years Proxima Centauri – Alpha Centauri...
The roAp stars are sometimes referred to as rapidly oscillating α2 CanumVenaticorum variables. Both the roAp stars and some α2 CVn variables lie on the...
were detected later. SN 2002bj Lupus +14.7 160,000,000 IIn NGC 1821 AMCanumVenaticorum-type outburst. SN 2003fg Boötes 4,000,000,000 Ia anonymous galaxy...
outbursts during the dim state. They may be a subclass of polars. AMCanumVenaticorum These are cataclysmic variables both of whose components are white...
Sujan; Taam, Ronald E. (2011-09-02). "Theoretical Spectra of the AmCanumVenaticorum Binary System SDSS J0926+3624: Effects of Irradiation Onto the Donor...
helium star losing mass to a white dwarf. It is an example of the AMCanumVenaticorum (AM CVn) type of cataclysmic variable stars. Patterson, Joseph; Walker...
HR 5110, also known as BH CanumVenaticorum, is a binary star system in the northern constellation of Canes Venatici. It is visible to the naked eye with...
Bildsten et al. had predicted this category of explosion would occur in AMCanumVenaticorum star binary systems. NGC 1821 is an irregular galaxy categorized...
P = 0.21 d RX J0806.3+1527 HM 08h 06m 22.95s +15° 27′ 31.1″ 160 AMCanumVenaticorum star AK Cnc AK 08h 55m 21.18s +11° 18′ 15.3″ SU UMa variable CC Cnc...
6.67 and 6.76 in a cycle of 69.51 days. It is classified as an α2 CanumVenaticorum variable. The HN Andromedae system is triple, as seen in periodic...
and 63 times that of the Sun. Alpha Piscium is catalogued as an α2 CanumVenaticorum variable, a type of variable star where the brightness changes are...
spectrum. This is a suspected variable star of the type known as Alpha² CanumVenaticorum. There is a magnitude 9.86 companion star at an angular separation...
HD 224801, also known as CG Andromedae, is an Alpha2 CanumVenaticorum variable star in the constellation Andromeda. Located approximately 188 parsecs...
63 Andromedae (abbreviated 63 And) is an Alpha2 CanumVenaticorum (α2 CVn) variable star in the constellation Andromeda. Its variable star designation...
binary viewed from nearly pole-on. This star is classified as an α2 CanumVenaticorum type variable star and its brightness varies by 0.03 magnitudes. It...
anomalies of silicon, strontium, and mercury in the spectrum. It is an α2 CanumVenaticorum variable with an amplitude of 0.05 magnitude in the B (blue) band...
vary by less than 0.5 magnitudes (70% change in luminosity). Alpha2 CanumVenaticorum (α2 CVn) variables are main-sequence stars of spectral class B8–A7...
also known as HR 369 in the Bright Star Catalogue) is an Alpha2 CanumVenaticorum variable in the constellation Andromeda. Its maximum apparent visual...
also been classified as a mercury-manganese star. V686 CrA is an α2 CanumVenaticorum variable that ranges from 5.25 to 5.41 within 3.674 days. It has been...
visibility to the naked eye even under good viewing conditions. An Alpha2 CanumVenaticorum variable, it varies in brightness by 0.012 magnitude every 0.66 days...
(hA7) and metal (mA7) absorption lines of an A7 star. It is an Alpha2 CanumVenaticorum-type variable with magnitude ranging from 4.62 down to 4.67 over a...
mercury-manganese star. The star is tentatively catalogued as an Alpha2 CanumVenaticorum variable, with brightness variations of just 0.01 magnitudes. The...