Asteroseismology across the HR diagram
arXiv:astro-ph/0702304 · doi:10.1007/978-3-540-75485-5_34
Abstract
High precision spectroscopy provides essential information necessary to fully exploit the opportunity of probing the internal structure of stars using Asteroseismology. In this work we discuss how Asteroseismology combined with High Precision Spectroscopy can establish a detailed view on stellar structure and evolution of stars across the HR diagramme.
6 pages, 2 figures - to appear in Precision Spectroscopy in Astrophysics, (Eds) L. Pasquini, M. Romaniello, N.C. Santos, and A. Correia, ESO Astrophysics Symposia, 2007
References in corpus (8)
- An asteroseismic study of the beta Cephei star beta Canis Majoris
- Solar-like oscillations in the metal-poor subgiant nu Indi: constraining the mass and age using asteroseismology
- Models of Procyon A including seismic constraints
- Asteroseismic Diagnostics of Stellar Convective Cores
- Pulsating young brown dwarfs
- Space and Ground Based Pulsation Data of Eta Bootis Explained with Stellar Models Including Turbulence
- A multisite photometric campaign on the Pre-Main-Sequence delta Scuti pulsator IP Per
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Cited by in corpus (12)
- Solar-like Oscillations (Invited Review)
- Asteroseismic determination of helium abundance in stellar envelopes
- Ellipsoidal Variability and Long Secondary Periods in MACHO Red Giant Stars
- Asteroseismological studies of three Beta Cephei stars: IL Vel, V433 Car and KZ Mus
- Asteroseismic Signatures of Helium gradients in Main-Sequence A Stars ; Application to the roAp Star HD60435
- Asteroseismic modelling of the metal-poor star Tau Ceti
- Variability in mode amplitudes in the rapidly oscillating Ap star HR 1217
- The 2003-4 multisite photometric campaign for the Beta Cephei and eclipsing star 16 (EN) Lacertae with an Appendix on 2 Andromedae, the variable comparison star
- Seismic analysis of 70 Ophiuchi A: A new quantity proposed
- Solar-type Variables
- Dynamic Tides in Close Binaries
- Towards a theory of rapidly oscillating Ap stars