T Pyxidis (T Pyx) is a recurrent nova and nova remnant in the constellation Pyxis. It is a binary star system and its distance is estimated at 4,783 parsecs...
12 KB (1,128 words) - 03:41, 17 July 2024
Nova Persei 1901 or the energies remaining in the expanding bubbles like T Pyxidis. Most novae require a close binary system, with a white dwarf and a main...
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M. (2010-01-01). "The Nova Shell and Evolution of the Recurrent Nova T Pyxidis". The Astrophysical Journal. 708 (1): 381–402. arXiv:0906.0933. Bibcode:2010ApJ...
26 KB (1,872 words) - 04:25, 16 September 2024
explosion. T Coronae Borealis is one of a handful of stars called recurrent novae, which include T Pyxidis and U Scorpii. An outburst of T Coronae Borealis...
55 KB (6,381 words) - 09:14, 29 August 2024
Committee of Photographic Magnitudes in 1913. In 1913, Leavitt discovered T Pyxidis, a recurrent nova in the constellation Pyxis, and one of the most frequent...
30 KB (3,013 words) - 04:55, 19 June 2024
the dense atmosphere of the white dwarf after each ignition, as in the star T Coronae Borealis. Under certain conditions, mass accretion can eventually...
28 KB (3,022 words) - 22:00, 5 September 2024
supernovae Variable star A higher magnitude means a lower brightness. i.e. T Aurigae (+3.8) was a brighter nova than HR Lyrae (+6.5) Prialnik, Dina. "Novae"...
11 KB (683 words) - 20:23, 10 September 2023
Alpha Pyxidis, Latinised from α Pyxidis, is a giant star in the constellation Pyxis. It has a stellar classification of B1.5III and is a Beta Cephei variable...
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about 4 to 9 magnitudes, repeating every 10 to 80 years. Examples include T Pyxidis and RS Ophiuchi. Dwarf novae Dwarf novae, or U Geminorum stars, are cataclysmic...
11 KB (994 words) - 20:06, 19 July 2024