YZ Reticuli (section VY Sculptoris type)
Reticulum discovered on July 15, 2020. Previously it was known as a VY Sculptoris type object with the designation MGAB-V207. The variability of the object...
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Super soft X-ray source (redirect from VY Sculptoris variable)
cessation of Ṁ from the secondary. These are the VY Scl-type stars or anti-dwarf novae. V751 Cyg (BB, MW) is a VY Scl CV, has a bolometric luminosity of 6.5...
20 KB (2,508 words) - 01:33, 28 November 2023
ISBN 978-0-387-79945-2. Hameury, Jean-Marie; Lasota, Jean-Pierre (October 4, 2002). "VY Sculptoris stars as magnetic CVs". Astronomy and Astrophysics. 394 (1): 231–239...
12 KB (1,009 words) - 16:31, 6 October 2024
consisting of a red dwarf and a white dwarf. Originally classified as a VY Sculptoris star due to spending most time at maximum brightness, since around 1979...
68 KB (7,573 words) - 23:23, 16 July 2024
Camelopardalis (UGZ) type, it has shown low-luminosity periods typical of VY Sculptoris stars. However, for most of the time it varies from an apparent visual...
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largest-known supergiant stars in the Milky Way are class M stars, such as VY Canis Majoris, VV Cephei, Antares, and Betelgeuse. Furthermore, some larger...
105 KB (11,508 words) - 10:59, 6 October 2024