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- Volume 88 - Année 2019
- Actes de colloques
- 2nd Belgo-Indian Network for Astronomy & Astrophys...
- Asteroseismology in the BINA context
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Anwesh
Mazumdar, Bhaswati
Mookerjea & Pritesh
Ranadive Asteroseismology in the BINA context
(Volume 88 - Année 2019 — Actes de colloques — 2nd Belgo-Indian Network for Astronomy & Astrophysics (BINA) workshop - October 2018 - Brussels, Belgium)
Article
Mots-clés : astrosismologie, étoiles de type solaire, photométrie, couleur, temperature effective
Abstract
The scope of asteroseismic studies within the Belgo-Indian Network for Astronomy and astrophysics (BINA) is explored. The main strands of current research in asteroseismology of solar-type stars are outlined. While it is obvious that it would be difficult to match the quality of the space-based seismic data on such stars with ground-based telescopes, the possibility of contribution to supplemental non-seismic data is considered. New calibrations of colour-temperature relations using archival data are presented. It is proposed that with similar calibrations with BINA-based photometric data in the future, it would be possible to provide accurate estimates of effective temperatures of solar-type stars that would be useful in asteroseismology of such stars.
Keywords : asteroseismology, solar-type stars, photometry, colour, effective temperature
Om dit artikel te citeren:
Anwesh Mazumdar, Bhaswati Mookerjea & Pritesh Ranadive, «Asteroseismology in the BINA context», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 88 - Année 2019, Actes de colloques, 2nd Belgo-Indian Network for Astronomy & Astrophysics (BINA) workshop - October 2018 - Brussels, Belgium, 121-127 URL : https://popups.uliege.be/0037-9565/index.php?id=8741.
Homi Bhabha Centre for Science Education (TIFR), V. N. Purav Marg, Mumbai 400088, India.
Dept. of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India.
Homi Bhabha Centre for Science Education (TIFR), V. N. Purav Marg, Mumbai 400088, India.