Seismic Inversions for White Dwarf Stars
2002 ◽
Vol 185
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pp. 606-607
Keyword(s):
The Sun
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AbstractInversion methods have been used successfully for the Sun. The stars with the next richest set of observed frequencies are the white dwarfs. We consider here the viability of numerical inversions for these stars. We find that, while the number of presently observed modes in the white dwarf GD 358 is too small for structural inversions, such inversions would be possible if the frequencies of all modes with 1 ≤ l ≤ 3 were observed. This is possible for space observations by e.g. Eddington.
2017 ◽
Vol 45
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pp. 1760023
Keyword(s):
2009 ◽
Vol 5
(H15)
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pp. 370-370
Keyword(s):
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1978 ◽
Vol 80
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pp. 117-120
Keyword(s):
1971 ◽
Vol 42
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pp. 67-76
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Keyword(s):
1989 ◽
Vol 114
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pp. 384-387
Keyword(s):
2002 ◽
Vol 185
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pp. 608-609
Keyword(s):
1993 ◽
Vol 139
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pp. 116-116
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2021 ◽
pp. 2140006
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