Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-19T05:03:15.080Z Has data issue: false hasContentIssue false
  • English
  • Français

Stephi: A New Approach to δ Scuti Asteroseismology

Published online by Cambridge University Press:  12 April 2016

J.A. Belmonte ,
T. Roca Cortés ,
I. Vidal ,
F.X. Schmider ,
E. Michel ,
A. Baglin ,
M. Chevreton ,
M. Auvergne ,
A. Man-Geney  and
M.J. Goupil
...Show all authors
J.A. Belmonte
Affiliation:
Instituto de Astrofísica de Canarias, 38200, La Laguna, Tenerife, Spain
T. Roca Cortés
Affiliation:
Instituto de Astrofísica de Canarias, 38200, La Laguna, Tenerife, Spain
I. Vidal
Affiliation:
Instituto de Astrofísica de Canarias, 38200, La Laguna, Tenerife, Spain
F.X. Schmider
Affiliation:
Instituto de Astrofísica de Canarias, 38200, La Laguna, Tenerife, Spain
E. Michel
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon, France.
A. Baglin
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon, France.
M. Chevreton
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon, France.
M. Auvergne
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon, France.
A. Man-Geney
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon, France.
M.J. Goupil
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon, France.
G. Massacrier
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon, France.
T. Serre
Affiliation:
Observatoire de Paris-Meudon, 92195 Meudon, France.
M. Álvarez
Affiliation:
Instituto de Astronomía de la U.N.A.M., Ap. Postal 877, Ensenada, BC, Mexico.
S.Y. Jiang
Affiliation:
Beijing Observatory, Chinese academy of Sciences, Beijing, China.
Y.Y. Liu
Affiliation:
Beijing Observatory, Chinese academy of Sciences, Beijing, China.
J.N. Fu
Affiliation:
Beijing Observatory, Chinese academy of Sciences, Beijing, China.
N. Dolez
Affiliation:
Observatoire Midi-Pyrénées, 31400 Toulouse, France.
J.P. Sareyan
Affiliation:
Departement d’Astrophysique, Université de Nice, 06034 Nice, France.
J.C. Valtier
Affiliation:
Departement d’Astrophysique, Université de Nice, 06034 Nice, France.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The STEPHI network (STEllar PHotometry International) is a multinational cooperation stablished in order to get as perfect data as possible on several δ Scuti stars, within a reasonable period of time. STEPHI is currently integrated by nearly 15 people, belonging to the first four institutions cited above. However, astronomers of other institutions have eventually contributed to the network. The idea was born in 1986 and the network has been working to full operation since August 1989. A campaign, observing one or two δ Scuties is normally undertaken every 15 months. They are usually order of three weeks long, avoiding full-moon periods. Up to now, four campaigns have been performed, the last ending February 1992.

Very good outcomes on five δScuties [63 Herculis in June 1987 (Belmonte et al, 1991), GX Pegasi in September 1989 (Michel et al, 1992a), v650 Tauri in November 1990 (Belmonte and Michel, 1991; Michel et al, 1992b) and, finally, BN Cancri and BU Cancri in February 1992] have been obtained. Indeed, some very useful aditional information on comparison stars (see e.g. Belmonte et al, 1990) and sky conditions (transparency, brightness, scintillation, etc..) has been obtained as well. Aditionally, some key information about mostly all multiperiodic (four or more periods) δ Scuti stars studied up to March 1992, with good quality data, is presented in this report.

Type
VIII. Asteroseismology: observation
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 739 - 742
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Balona, L.A. & Stobie, R.S., 1980. M.N.R.A.S. 190, 931.CrossRefGoogle Scholar
Belmonte, et al, 1990. A&A, 231, 303.Google Scholar
Belmonte, et al, 1991. A&A, 246, 71.Google Scholar
Belmonte, J.A. & Michel, E., 1991. Delta Scuti News. 3, 16.Google Scholar
BogKa, P. & Conconi, P., 1985. A&A, 149, 15.Google Scholar
Bossi, et al, 1982. Astrophys. Spa Sci., 85, 25.Google Scholar
Breger, M., 1990. A&A, 240, 308.Google Scholar
Breger, et al, 1987. A&A, 175, 117.Google Scholar
Breger, et al, 1989. A&A, 214, 209.Google Scholar
Breger, et al, 1990. A&A, 231, 56.Google Scholar
Kovàcs, G., 1981. Act. Astron., 31, 75.Google Scholar
Lampens, S.R. & Rufener, F., 1990. A&A Sup., 83, 145.Google Scholar
Mantegazza, et al, 1992. This proceedings.Google Scholar
Mc Namara, B.J. & Horan, S.J., 1984. AP. J., 282, 741.Google Scholar
Mc Namara, et al, 1989. In IAU Col. Ill: the Use of Pulsating Stars in Fundamental Problems of Astronomy. Schmidt, E.G. (ed). Cambridge Univ. Press, 276.Google Scholar
Michel, et al, 1992a. A&A, 255, 139.Google Scholar
Michel, et al, 1992b. This proceedings.Google Scholar
Ostermann, et al, 1991. A&A, 245, 543.Google Scholar
Rucinski, S.M., 1978. Act. Astron., 28, 545.Google Scholar
Stobie, et al, 1977. M.N.R.A.S., 179, 389.Google Scholar