1998BaltA...7...11K


Query : 1998BaltA...7...11K

1998BaltA...7...11K - Baltic Astronomy, 7, 11-20 (1998/March-0)

What can we learn from WET about how to make white dwarfs?

KAWALER S.D.

Abstract (from CDS):

Aside from the many things we have learned about stellar pulsation from the pulsating white dwarfs, seismic study of their interiors feeds back into the theory of stellar evolution. In particular, from pulsating white dwarfs has come a much better understanding of the processes by which white dwarfs are made. In this brief review, I describe what the hot pulsating white dwarfs have taught us about white dwarf interiors, and how this knowledge has tested the theory of stellar evolution. I also discuss some future prospects for continued discoveries in stellar evolution through study of the pulsators.

Abstract Copyright: ∼

Journal keyword(s): stars: white dwarfs, oscillations, evolution

CDS comments: RX J2117 = RX J2117.1+3412

Simbad objects: 8

goto View the references in ADS

Number of rows : 8
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 NGC 246 PN 00 47 03.3420341616 -11 52 18.971126076 10.15 11.52 11.76 12.18   PG1159 489 0
2 PG 0122+200 WD* 01 25 22.5121704552 +20 17 56.963079924   16.2   16.9   DOZ.7 117 0
3 NGC 1501 PN 04 06 59.3920909320 +60 55 14.278542024   15.17 13.0     [WO4] 314 1
4 NGC 2671 OpC 08 46 17.0 -41 53 22     11.6     ~ 36 0
5 V* GW Vir WD* 12 01 45.9731868264 -03 45 40.628670300   14.87 15.04     DOQZ1 505 0
6 GD 358 WD* 16 47 18.3925183824 +32 28 32.862804384 12.511 13.530 13.653 13.752 13.852 DB2 364 0
7 MWP 1 PN 21 17 08.2817782392 +34 12 27.415995372   12.731 13.082 13.379   PG1159 199 0
8 V* IR Peg WD* 21 34 08.2124719240 +06 50 57.662044329   16.15       PG1159 122 0

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