• Thumbnail for Dwarf nova
    A dwarf nova (pl. novae), or U Geminorum variable, is one of several types of cataclysmic variable star, consisting of a close binary star system in which...
    7 KB (701 words) - 22:14, 21 February 2025
  • Thumbnail for Nova
    star (hence the name "nova", Latin for "new") that slowly fades over weeks or months. All observed novae involve white dwarfs in close binary systems...
    29 KB (3,093 words) - 01:41, 15 March 2025
  • Thumbnail for Cataclysmic variable star
    the inner edge of disc falls onto the surface of the white dwarf primary. A classical nova outburst occurs when the density and temperature at the bottom...
    12 KB (1,009 words) - 23:13, 4 March 2025
  • its Roche lobe so that matter is transferred to the white dwarf and accumulates until a nova-like outburst occurs, caused by ignition of thermonuclear...
    3 KB (373 words) - 18:31, 3 August 2024
  • Thumbnail for V339 Delphini
    the white dwarf nova progenitor acquired from its companion star. The nova system is thus a binary star, and a classical nova. The white dwarf is a carbon-oxygen...
    8 KB (683 words) - 10:59, 22 August 2024
  • Thumbnail for Brown dwarf
    could also exist brown dwarfs that merged with white dwarfs. The nova CK Vulpeculae might be a result of such a white dwarf–brown dwarf merger. The earliest...
    166 KB (18,155 words) - 22:24, 8 May 2025
  • Thumbnail for Luminous red nova
    at the predicted time. Binary star Cataclysmic variable star Dwarf nova Hypernova Nova Supernova Kulkarni, S. R.; Ofek, E. O.; Rau, A.; Cenko, S. B.;...
    10 KB (1,144 words) - 20:30, 12 May 2025
  • Thumbnail for WZ Sagittae
    WZ Sagittae (category Dwarf novae)
    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...
    10 KB (1,017 words) - 19:19, 7 May 2025
  • Thumbnail for Corvus (constellation)
    fourth planetary system is unconfirmed. TV Corvi is a dwarf nova—a white dwarf and brown dwarf in very close orbit. In the Babylonian star catalogues...
    51 KB (6,172 words) - 23:25, 1 March 2025
  • Thumbnail for BW Sculptoris
    BW Sculptoris (category Dwarf novae)
    Sge-type dwarf nova and a candidate period bouncer. The binary consists of a white dwarf and a brown dwarf donor that orbits the white dwarf every 78...
    7 KB (703 words) - 04:50, 2 March 2025
  • Thumbnail for Messier 5
    could shed light on some hypothetical particles such as the axion. A dwarf nova has also been observed in this cluster. Globular cluster Messier 5 in...
    10 KB (895 words) - 22:47, 7 May 2025
  • Thumbnail for Leo Minor
    clock. SX Leonis Minoris is a dwarf nova of the SU Ursae Majoris type that was identified in 1994. It consists of a white dwarf and a donor star, which orbit...
    41 KB (3,905 words) - 04:43, 4 May 2025
  • Thumbnail for Coma Berenices
    ultraviolet, the white dwarf HZ 43, was discovered in Coma Berenices. In 1995, there was a very rare outburst of the WZ Sagittae-type dwarf nova AL Comae Berenices...
    64 KB (6,974 words) - 22:25, 3 May 2025
  • Thumbnail for GK Persei
    GK Persei (redirect from Nova Persei 1901)
    seems to have changed from a classical nova like Nova Aquilae 1918 to something resembling a typical dwarf nova-type cataclysmic variable star. Surrounding...
    10 KB (908 words) - 06:38, 7 October 2024
  • Thumbnail for Cygnus (constellation)
    2030+ 375. Cygnus is also home to several variable stars. SS Cygni is a dwarf nova which undergoes outbursts every 7–8 weeks. The system's total magnitude...
    52 KB (5,898 words) - 00:30, 4 May 2025
  • the term compact object (or compact star) refers collectively to white dwarfs, neutron stars, and black holes. It could also include exotic stars if such...
    20 KB (2,589 words) - 22:40, 1 March 2025
  • Thumbnail for Lyra
    most peculiar systems in Lyra is MV Lyrae, a nova-like star consisting of a red dwarf and a white dwarf. Originally classified as a VY Sculptoris star...
    68 KB (7,584 words) - 22:17, 3 May 2025
  • Thumbnail for Astronomical object
    active galactic nucleus. Galaxies can also have satellites in the form of dwarf galaxies and globular clusters. The constituents of a galaxy are formed...
    29 KB (1,595 words) - 04:18, 3 May 2025
  • Thumbnail for Gemini (constellation)
    magnitude 4.8 and the secondary is a yellow star of magnitude 7.8. U Gem is a dwarf nova type cataclysmic variable discovered by J. R. Hind in 1855. M35 (NGC 2168)...
    20 KB (2,270 words) - 02:22, 23 March 2025
  • Thumbnail for TV Corvi
    TV Corvi (category Dwarf novae)
    TV Corvi, also known as Tombaugh's Star, is a dwarf nova of the SU Ursae Majoris type in the constellation Corvus that was first discovered by accident...
    7 KB (691 words) - 19:33, 24 October 2024
  • Thumbnail for Hydrus
    Gamma is the VW Hydri, a dwarf nova of the SU Ursae Majoris type. It is a close binary system that consists of a white dwarf and another star, the former...
    29 KB (3,090 words) - 14:30, 2 May 2025
  • Thumbnail for Triangulum Australe
    Australis, a dwarf nova of the SU Ursae Majoris type, was first noticed in 1978 and officially described in 1980. It consists of a white dwarf and a donor...
    33 KB (3,326 words) - 01:39, 28 February 2025
  • Thumbnail for SN 393
    lengthy duration suggests the source was a supernova. However, a classical nova is not excluded as possibility. Before 1975, the observation made by the...
    11 KB (1,164 words) - 01:02, 23 April 2025
  • Thumbnail for Time-domain astronomy
    term is used for violent deep-sky events, such as supernovae, novae, dwarf nova outbursts, gamma-ray bursts, and tidal disruption events, as well as gravitational...
    12 KB (1,324 words) - 06:35, 9 March 2025
  • Thumbnail for Red dwarf
    A red dwarf is the smallest kind of star on the main sequence. Red dwarfs are by far the most common type of fusing star in the Milky Way, at least in...
    36 KB (4,265 words) - 18:28, 17 May 2025
  • Thumbnail for U Geminorum
    U Geminorum (category Dwarf novae)
    is an archetypal example of a dwarf nova. The binary star system consists of a white dwarf closely orbiting a red dwarf. Every few months it undergoes...
    9 KB (819 words) - 06:19, 6 January 2025
  • Thumbnail for Superhump
    Superhump (category Dwarf novae)
    periods slightly less than the orbital period. Superhumps can occur in dwarf nova systems in which the donor star (mass-losing star) has a mass that is...
    3 KB (399 words) - 18:55, 13 September 2024
  • be prone to instability leading to dwarf nova outbursts: a portion of the disk material falls onto the white dwarf, the cataclysmic outbursts occur when...
    20 KB (2,501 words) - 15:38, 6 March 2025
  • that are known to have occurred in 2019. A nova is an energetic astronomical event caused by a white dwarf accreting matter from a star it is orbiting...
    10 KB (422 words) - 12:29, 6 February 2024
  • Thumbnail for Black dwarf
    A black dwarf is a theoretical stellar remnant, specifically a white dwarf that has cooled sufficiently to no longer emit significant heat or light. Because...
    11 KB (1,252 words) - 21:52, 18 May 2025