Evolutionary and pulsational models of metal-poor subdwarfs
Metal-poor subdwarfs (MPSDs) are probably the Sun's oldest neighbours and are almost certainly low-amplitude p-mode pulsators, like the Sun. One of the goals of the MOST Space Telescope project (due for launch in 2002 - 2003) is to detect MPSD oscillations and apply asteroseismology to refin...
Main Author: | Shkolnik, Evgenya |
---|---|
Format: | Others |
Language: | English |
Published: |
2009
|
Online Access: | http://hdl.handle.net/2429/10973 |
Similar Items
-
Evolutionary and pulsational models of metal-poor subdwarfs
by: Shkolnik, Evgenya
Published: (2009) -
A survey of hot subdwarf pulsators in ω Cen
by: Catelan M., et al.
Published: (2013-03-01) -
Erratum to: A survey of hot subdwarf pulsators in ω Cen
by: Bono G., et al.
Published: (2013-04-01) -
New observations and asteroseismic analysis of the subdwarf B pulsator PG 1219+534
by: Van Grootel Valérie, et al.
Published: (2018-03-01) -
ε-mechanism driven pulsations in hot subdwarf stars with mixed H-He atmospheres
by: Battich Tiara, et al.
Published: (2017-12-01)