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Autor:
Wei-Chun Jao, Todd J. Henry, Russel J. White, Azmain H. Nisak, Hodari-Sadiki Hubbard-James, Leonardo A. Paredes, Vanders B. Lewis Jr.
Publikováno v:
The Astronomical Journal, Vol 166, Iss 2, p 63 (2023)
Since identifying the gap in the H-R Diagram (HRD) marking the transition between partially and fully-convective interiors, a unique type of slowly pulsating M dwarf has been proposed. These unstable M dwarfs provide new laboratories in which to unde
Externí odkaz:
https://doaj.org/article/ef04706df2214845aff5564952e2eaa3