Pulsating Hot Subdwarf Stars

Hot subdwarf stars are core helium-burning objects, located at the hot end of the horizontal branch, and therefore, they are also known as Extreme Horizontal Branch stars. We can divide them into two large groups, of spectral types B and O, depending on their effective temperature. Each spectroscopi...

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Detalles Bibliográficos
Autor principal:	Romero, Alejandra Daniela
Formato:	Objeto de conferencia
Lenguaje:	Inglés
Publicado:	2019
Materias:	Ciencias Astronómicas asteroseismology instabilities stars: oscillations stars: interiors
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/167764
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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