Published October 2008
| Version v1
Journal article
Nonadiabatic asteroseismology of GW Vir stars
- 1. Institut for Fysik og Astronomi, Aarhus Universitet Ny Munkegade, Bygn. 1520, 8000 Arhus-C (Denmark)
- 2. Departement de physique Universite de Montreal, C.P. 6128, Succ. centre-ville, Montreal (Quebec) H3C 3J7 (United States)
Description
We present and explore a new method involving a nonadiabatic stability calculation to determine the position of the GW Vir band in the log g - Teff diagram. With this method, we calculate the position of two GW Vir stars, PG 1159-035, log g = 6.80, Teff = 144, 500 K and PG 1707+427, log g = 7.38, Teff = 81, 500 K. The results are consistent with and complementary to the spectroscopic determination of atmospheric parameters and the chemical compositions of these stars.
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/118/1/012069Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 118
- Journal Issue
- 1
- Journal Page Range
- [6 p.]
- ISSN
- 1742-6596
Conference
- Title
- 2. HELAS international conference on helioseismology, asteroseismology and MHD connections
- Dates
- 20-24 Aug 2007
- Place
- Goettingen (Germany)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41036365
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; CHEMICAL COMPOSITION; DIAGRAMS; SEISMOLOGY; SPECTROSCOPY; STABILITY; STARS
- Descriptors DEC
- INFORMATION; PHYSICS