2014MNRAS.443.3477C


Query : 2014MNRAS.443.3477C

2014MNRAS.443.3477C - Mon. Not. R. Astron. Soc., 443, 3477-3485 (2014/October-1)

Asteroseismology of DAV star EC14012-1446, mode identification and model fittings.

CHEN Y.H. and LI Y.

Abstract (from CDS):

EC14012-1446 was observed by Handler et al. in 2004 April, June, 2005 May, and 2007 April, and by Provencal et al. in 2008. We review the observations together and obtain 34 independent frequencies. According to the frequency splitting and the asymptotic period spacing law, we identify 6 l = 1 modes, 4 l = 2 modes, 5 l = 3 modes, 10 l = 1 or 2 modes. Grids of white dwarf models are generated by wdec with H, He, C, O diffusion in a four-parameter space. The core compositions are directly from white dwarf models generated by mesa. The best-fitting model has M* = 0.710 M☉, Teff = 12 200 K, log(MHe/M*) = -2.5, log(MH/M*) = -7.0, log g = 8.261, and φ = 3.185 s. There are four, two, and one modes identified as trapped in H envelope for observed l = 1, 2, and 3 modes, respectively. Trapped modes jump the queue of uniform period spacing.

Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): asteroseismology - stars: individual: EC14012-1446 - white dwarfs

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 EC 14012-1446 WD* 14 03 57.1692959280 -15 01 10.577565696   15.86 15.67 15.89   DA4.1 63 0
2 V* ZZ Psc WD* 23 28 47.6365087803 +05 14 54.235051503   13.217   13.106   DA4.1 536 0

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