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The Delta Scuti Network: Steps Towards Successful Asteroseismology of Delta Scuti Stars

Published online by Cambridge University Press:  12 April 2016

W. Zima ,
M. Breger ,
K. Bischof ,
F. Rodler ,
A. Stankov ,
A. A. Pamyatnykh ,
V. Antoci ,
D. Lorenz ,
M. Sperl  and
R. Zechner
...Show all authors
W. Zima
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
M. Breger
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
K. Bischof
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
F. Rodler
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
A. Stankov
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
A. A. Pamyatnykh
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
V. Antoci
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
D. Lorenz
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
M. Sperl
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
R. Zechner
Affiliation:
Institut für Astronomie, Türkenschanzstr. 17, A-1180 Wien, Austria, zima@astro.univie.ac.at
R. Garrido
Affiliation:
Instituto de Astrofisica de Andalucia, CSIC, Apdo. 3004, E-18080 Granada, Spain
M. Wood
Affiliation:
Dept. of Physics and Space Science, Florida Institute of Technology, Melbourne, FL 32901, U.S.A.
G. Handler
Affiliation:
SAAO, P.O. Box 9, Observatory 7935, Cape Town, South Africa
R.R. Shobbrook
Affiliation:
School of Physics, University of Sydney2006, Australia

Abstract

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The Delta Scuti Network (DSN) is a collaboration of astronomers all around the globe who study and observe short-period variables. The field of scientific research includes high-precision photometric and Spectroscopic global campaigns, mode identification techniques, and asteroseismological pulsation modeling. We present results for three stars that are receiving the most attention at the moment: 4 CVn, BI CMi, and 44 Tau. Our results demonstrate that a large number of simultaneously excited nonradial oscillations in stars on and above the main sequence can be detected by conventional means.

Type
Part 6. Asteroseismology from Space and from the Ground
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 598 - 599
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

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