Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-29T10:36:13.394Z Has data issue: false hasContentIssue false
  • English
  • Français

First Results of the 17th DSN Campaign: Photometry of XX Pyx

Published online by Cambridge University Press:  12 April 2016

T. Arentoft ,
G. Handle ,
R. R. Shobbrook ,
M. A. Wood ,
L. Crause ,
P. Crake ,
F. Podmore ,
A. Habanyama ,
T. Oswalt  and
P. V. Birch
...Show all authors
T. Arentoft
Affiliation:
Vrije Universiteit Brussel (VUB), Pleinlaan 2, B-1050 Brussels, Belgium
G. Handle
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstraße 17, A-1180 Wien, Austria South African Astronomical Observatory, P.O. Box 9, Observatory 7935, South Africa
R. R. Shobbrook
Affiliation:
P. O. Box 518, Coonabarabran, N.S.W 2357, Australia
M. A. Wood
Affiliation:
Dept. of Physics and Space Sciences, Florida Institute of Technology, 150 W. University Blvd., Melbourne, FL 32901, USA
L. Crause
Affiliation:
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa
P. Crake
Affiliation:
Perth Observatory, Walnut Rd., Bickley, Western Australia 6076, Australia
F. Podmore
Affiliation:
Physics Department, University of Zimbabwe, P.O. Box MP167, Mt Pleasant, Harare, Zimbabwe
A. Habanyama
Affiliation:
Department of Physics, University of Zambia, P.O. Box 32379, Lusaka, Zambia
T. Oswalt
Affiliation:
Dept. of Physics and Space Sciences, Florida Institute of Technology, 150 W. University Blvd., Melbourne, FL 32901, USA
P. V. Birch
Affiliation:
Perth Observatory, Walnut Rd., Bickley, Western Australia 6076, Australia
G. Lowe
Affiliation:
Perth Observatory, Walnut Rd., Bickley, Western Australia 6076, Australia
C. Sterken
Affiliation:
Vrije Universiteit Brussel (VUB), Pleinlaan 2, B-1050 Brussels, Belgium
P. Meintjes
Affiliation:
Physics Department, University of the Orange Free State, Bloemfontein 9300, South Africa
J. Brink
Affiliation:
Physics Department, University of the Orange Free State, Bloemfontein 9300, South Africa
C. F. Claver
Affiliation:
National Optical Astronomy Observatories, P. O. Box 26732, Tucson, AZ 85726-6732, USA
R. Medupe
Affiliation:
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa
J. A. Guzik
Affiliation:
Los Alamos National Laboratory, XTA, MS B220, Los Alamos, NM 87545-2345, USA
T. E. Beach
Affiliation:
University of New Mexico, Los Alamos, 4000 University Drive, Los Alamos, NM 87544, USA
P. Martinez
Affiliation:
South African Astronomical Observatory, P.O. Box 9, Observatory 7935, South Africa
E. M. Leibowitz
Affiliation:
Wise Obs., Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv 69978, Israel
P. A. Ibbetson
Affiliation:
Wise Obs., Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv 69978, Israel
T. Smith
Affiliation:
Perth Observatory, Walnut Rd., Bickley, Western Australia 6076, Australia
B. N. Ashoka
Affiliation:
Indian Space Research Organization, Technical Physics Division, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
N. E. Raj
Affiliation:
Indian Space Research Organization, Technical Physics Division, ISRO Satellite Centre, Airport Road, Bangalore 560 017, India
D. W. Kurtz
Affiliation:
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa
L. A. Balona
Affiliation:
South African Astronomical Observatory, P.O. Box 9, Observatory 7935, South Africa
J. E. S. Costa
Affiliation:
Instituto de Fisica, Universidade Federal do Rio Grande do Sul, 91501-970 Porto Alegre-RS, Brazil
M. Breger
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstraße 17, A-1180 Wien, Austria

Abstract

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.

We present the first results from multi-site observations of the δ Scuti star XX Pyx (CD–24°7599). The observations were carried out as the 17th run of the Delta Scuti Network. We collected 583 hr of B, V time-series photometry, resulting in a detection level (4σ) in the amplitude spectrum of 0.5 mmag. We detect 6 new pulsation frequencies, bringing the total number of frequencies known in this star up 19.

Type
Part 6. Variables Close to the Main Sequence
Information
International Astronomical Union Colloquium , Volume 176: The Impact of Large-Scale Surveys on Pulsating Star Research , 2000 , pp. 469 - 470
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Dziembowski, W.A. & Pamyatnykh, A.A. 1991, A&A, 248, Lll Google Scholar
Handler, G., Pikali, H., O’Donoghue, D., et al. 1997, MNRAS, 286, 303 Google Scholar
Handler, G., et al. 1999, in preparation for MNRASGoogle Scholar
Kjeldsen, H. & Frandsen, S. 1992, PASP, 104, 413 CrossRefGoogle Scholar
Nather, R.E., Winget, D.E., Clemens, J.C., et al. 1990, ApJ, 361, 309 Google Scholar