Hot Subdwarfs: Magnetic, Oscillatory and Other Physical Properties

Bibcode
2003Ap&SS.284..269O
Oreiro, R.; Pérez Hernández, F.; Manteiga, M.; Ulla, A.; González Pérez, J. M.; Zapatero Osorio, M. R.; GarcÍa López, R.; MacDonald, J.; Thejll, P.; Ferriz-Mas, A.; Saffer, R. A.; Elkin, V.
Referencia bibliográfica

Astrophysics and Space Science, v. 284, Issue 1, p. 269-272 (2003).

Fecha de publicación:
2003
Revista
Astrophysics and Space Science
Número de autores
12
Número de autores del IAC
3
Número de citas
0
Número de citas referidas
0
Descripción
Hot subdwarf stars (hot sds) are blue subluminous objects. Only a few determinations are available to date regarding the study of such aspects as rotation, microturbulent velocities or the magnetic nature of these objects. Over 26 sdBs are known to date to be multiperiodic rapid oscillators. This project presents preliminary results of new observations and models of a sample of pulsating and non-pulsating hot sds, including considerations on mass loss and eventual magnetic properties.
Tipo
Sin árbitro

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