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The rapidly pulsating subdwarf B star PG 1325+101 II. Structural parameters from asteroseismology
S. Charpinet*, R. Silvotti, A. Bonanno, G. Fontaine, P. Brassard, P. Chayer, E. M. Green, P. Bergeron, S. Bernabei, S. Leccia, H. Kjeldsen, R. Janulis, A. Frasca, R. Østensen, S. L. Kim, B. G. Park, X. Jiang, M. D. Reed, R. S. Patterson, K. M. Gietzen
*Corresponding author for this work
- Univ. Paul Sabatier Toulouse
- National Institute for Astrophysics
- Osservatorio Astrofisico di Catania
- University of Montreal
- Johns Hopkins University
- University of Victoria BC
- University of Arizona
- Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
- Aarhus University
- Vilnius University
- Isaac Newton Group of Telescopes
- Korea Astronomy and Space Science Institute
- CAS - National Astronomical Observatories
- Missouri State University
- Florida Institute of Technology
- Tel Aviv University
Research output: Contribution to journal › Article › peer-review
34
Scopus
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