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An AM Canum Venaticorum star (AM CVn star), is a rare type of cataclysmic variable star named after their type star, AM Canum Venaticorum. In these hot...

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...

"Genuine standstill in the AM CVn star CR Boo", arXiv:2302.04454 [astro-ph.SR] Isogai, K.; et al. (2015), "Research on AM CVn stars: ASASSN-14ei and CR...

of (3.5±0.5)×10−11 M☉/year and was proven to be a low-activity AM CVn star. The star system is showing signs of a high abundance of ionized nitrogen...

76°26′18″W / 36.9805°N 76.4384°W / 36.9805; -76.4384 USS Enterprise (CVN-65), formerly CVA(N)-65, is a decommissioned United States Navy aircraft...

In astronomy, the term compact object (or compact star) refers collectively to white dwarfs, neutron stars, and black holes. It could also include exotic...

eclipsing AM CVn star, as seen by ULTRACAM, arXiv:astro-ph/0610414 Sengupta, Sujan; Taam, Ronald E. (2011-09-02). "Theoretical Spectra of the Am Canum Venaticorum...

de Données astronomiques de Strasbourg. Retrieved 2007-01-03. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014....

oldest stars known HP Lib HP 15h 35m 53.08s −14° 13′ 12.2″ 13.65 Bpec AM CVn star and V777 Her variable, Vmax = 13.65m, Vmin = 13.8m, P = 0.013 d K2-315...

Cor Caroli is the constellation's brightest star, with an apparent magnitude of 2.9. La Superba (Y CVn) is one of the reddest naked-eye stars and one...

binary consisting of a dwarf helium star losing mass to a white dwarf. It is an example of the AM Canum Venaticorum (AM CVn) type of cataclysmic variable stars...

star PG 1346+082, or CR Boötis, an AM CVn star. The second target was V803 Centauri, a cataclysmic binary. The campaign was able to monitor the star systems...

variables, Luminous red novae, tidal disruption flares, compact binaries (AM CVn star), active galactic nuclei, transiting Extrasolar planets, RR Lyrae variable...

A carbon star (C-type star) is typically an asymptotic giant branch star, a luminous red giant, whose atmosphere contains more carbon than oxygen. The...

Retrieved 4 April 2012. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014. Ian Ridpath's Startales - Canis Venatici...

this was widely believed. Orbital periods can be less than an hour (for AM CVn stars), or a few days (components of Beta Lyrae), but also hundreds of thousands...

Caroli (α CVn), in Canes Venatici Denebola (β Leo), the tail of Leo Spica (α Vir), the wheat of Virgo Arcturus (α Boo), the brightest star in Boötes The...

first such case (discounting characters from mythology) was Cor Caroli (α CVn), named in the 17th century for Charles I of England. The remaining examples...

project naval airpower ashore. The aircraft carrier USS Abraham Lincoln (CVN-72) is the group's current flagship. Other units assigned as of 2024 include...

Wolf–Rayet stars, AM CVn stars, white dwarfs of spectral type WC, and transition stars like PG 1159. The first known extreme helium star, HD 124448, was...