A BRITE view on the massive O-type supergiant V973 Scorpii: hints towards internal gravity waves or sub-surface convection zones

Author:

Ramiaramanantsoa Tahina12ORCID,Ratnasingam Rathish3ORCID,Shenar Tomer4,Moffat Anthony F J12,Rogers Tamara M35,Popowicz Adam6,Kuschnig Rainer7,Pigulski Andrzej8,Handler Gerald9,Wade Gregg A10,Zwintz Konstanze11,Weiss Werner W7

Affiliation:

1. Département de physique, Université de Montréal, CP 6128, Succursale Centre-Ville, Montréal, Québec H3C 3J7, Canada

2. Centre de Recherche en Astrophysique du Québec (CRAQ), Montréal, Québec H3C 3J7, Canada

3. Department of Mathematics and Statistics, Newcastle University, Newcastle upon Tyne NE1 7RU, UK

4. Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Str 24/25, D-14476 Potsdam, Germany

5. Planetary Science Institute, Tucson, AZ 85721, USA

6. Instytut Automatyki, Politechnika Śla̧ska, Akademicka 16, PL-44-100 Gliwice, Poland

7. Institut für Astrophysik, Universität Wien, Türkenschanzstrasse 17, A-1180 Wien, Austria

8. Instytut Astronomiczny, Uniwersytet Wrocławski, Kopernika 11, PL-51-622 Wrocław, Poland

9. Nicolaus Copernicus Astronomical Center, Bartycka 18, PL-00-716 Warsaw, Poland

10. Department of Physics and Space Science, Royal Military College of Canada, Kingston, ON K7K 7B4, Canada

11. Institut für Astro- und Teilchenphysik, Universität Innsbruck, Technikerstrasse 25, A-6020 Innsbruck, Austria

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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