2002A&A...388..320W


Query : 2002A&A...388..320W

2002A&A...388..320W - Astronomy and Astrophysics, volume 388320-325 (2002/6-2)

Is the helium in the variable DB white dwarfs 3He?

WOLFF B., KOESTER D., MONTGOMERY M.H. and WINGET D.E.

Abstract (from CDS):

Asteroseismological analysis of the Whole Earth Telescope observations of the prototype variable DB white dwarf GD358 indicates a possible composition interface at a depth of about 10–6 M☉, which has usually been assumed to be the He/C transition zone. Such a small He layer is in contradiction with canonical evolution theory. Recently Montgomery & Winget (2000BaltA...9...23M) proposed that the transition zone is in fact the transition between the isotopes 3He and 4He, which are separated by the same sedimentation process separating hydrogen and helium in the DA white dwarfs. Therefore, the visible surface helium should be 3He. We have tested this hypothesis spectroscopically on another variable DB using the known relative isotopic shifts of up to 0.5Å. The spectra are consistent with a pure 4He atmosphere, making a 3He/4He interface a very unlikely explanation for the mode spectrum of GD 358.

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Journal keyword(s): stars: atmospheres - stars: interiors - stars: variables: general - stars: white dwarfs

Simbad objects: 6

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Number of rows : 6
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 GD 358 WD* 16 47 18.3925183824 +32 28 32.862804384 12.511 13.530 13.653 13.752 13.852 DB2 364 0
2 WG 34 WD* 17 30 23.0910906048 -57 55 25.713654528   15.23 15.27     DB 26 1
3 LS IV +06 2 HS* 18 06 55.4522031744 +06 21 57.246453756   12.11 12.14 12.32   sdBC1VHe39 37 0
4 BD-13 4937 Y*O 18 19 20.0319493560 -13 54 21.677384808 10.53 11.11 10.78     B1.5V 48 1
5 V* QU Tel WD* 20 09 40.1871967824 -52 25 15.864452508 14.51 15.25 15.03     DB2 60 1
6 LS IV +10 9 HS* 20 43 02.4781026312 +10 34 21.001039644 10.51 11.71 12.06     sdO 39 0

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