Title: Whole Earth Telescope observations of BPM 37093: A seismological test of crystallization theory in white dwarfs
Authors: Kanaan, A ×
Nitta, A
Winget, DE
Kepler, SO
Montgomery, MH
Metcalfe, TS
Oliveira, H
Fraga, L
da Costa, AFM
Costa, JES
Castanheira, BG
Giovannini, O
Nather, RE
Mukadam, A
Kawaler, SD
O'Brien, MS
Reed, MD
Kleinman, SJ
Provencal, JL
Watson, TK
Kilkenny, D
Sullivan, DJ
Sullivan, T
Shobbrook, B
Jiang, XJ
Ashoka, BN
Seetha, S
Leibowitz, E
Ibbetson, P
Mendelson, H
Meistas, EG
Kalytis, R
Alisauskas, D
O'Donoghue, D
Buckley, D
Martinez, P
van Wyk, F
Stobie, R
Marang, F
van Zyl, L
Ogloza, W
Krzesinski, J
Zola, S
Moskalik, P
Breger, M
Stankov, A
Silvotti, R
Piccioni, A
Vauclair, G
Dolez, N
Chevreton, M
Deetjen, J
Dreizler, S
Schuh, S
Perez, JMG
Ostensen, Roy
Ulla, A
Manteiga, M
Suarez, O
Burleigh, MR
Barstow, MA #
Issue Date: Mar-2005
Publisher: E d p sciences
Series Title: Astronomy & astrophysics vol:432 issue:1 pages:219-224
Abstract: BPM 37093 is the only hydrogen-atmosphere white dwarf currently known which has sufficient mass (similar to 1.1 M-.) to theoretically crystallize while still inside the ZZ Ceti instability strip (T-eff similar to 12 000 K). As a consequence, this star represents our first opportunity to test crystallization theory directly. If the core is substantially crystallized, then the inner boundary for each pulsation mode will be located at the top of the solid core rather than at the center of the star, affecting mainly the average period spacing. This is distinct from the "mode trapping" caused by the stratified surface layers, which modifies the pulsation periods more selectively. In this paper we report on Whole Earth Telescope observations of BPM 37093 obtained in 1998 and 1999. Based on a simple analysis of the average period spacing we conclude that a large fraction of the total stellar mass is likely to be crystallized.
ISSN: 0004-6361
Publication status: published
KU Leuven publication type: IT
Appears in Collections:Non-KU Leuven Association publications
× corresponding author
# (joint) last author

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