Issue |
A&A
Volume 442, Number 2, November I 2005
|
|
---|---|---|
Page(s) | 629 - 634 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20053640 | |
Published online | 07 October 2005 |
Discovery of fourteen new ZZ Cetis with SOAR
1
Instituto de Física, Universidade Federal do Rio Grande do Sul, 91501-900 Porto-Alegre, RS, Brazil e-mail: kepler@if.ufrgs.br
2
SOAR, Casilla 603, La Serena, Chile
3
Sloan Digital Sky Survey, Apache Pt. Observatory, PO Box 59, Sunspot, NM 88349, USA
4
Department of Astronomy and McDonald Observatory, University of Texas, Austin, TX 78712, USA
5
Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA
Received:
16
June
2005
Accepted:
21
July
2005
We report the discovery of fourteen new ZZ Cetis with the 4.1 m
Southern Astrophysical Research telescope, at Cerro Pachon, in Chile.
The candidates
were selected from the SDSS (Sloan Digital Sky Survey) DA white dwarf stars
with obtained from the
optical spectra fit, inside the ZZ Ceti instability strip.
Considering these stars
are multi-periodic pulsators and the pulsations propagate
to the nucleus of the star, they carry information on the
structure of the star and evolution of the progenitors.
The ZZ Cetis discovered
till 2003 are mainly within 100 pc from the Sun, and probe only
the solar vicinity. The recently discovered ones, and those
reported here, may sample a distinct population as they were
selected mainly perpendicular to the galactic disk and
cover a distance up to ≈
pc.
Key words: stars: white dwarf / stars: variables: general / stars: oscillations
© ESO, 2005
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