Proceedings Paper
Simulating interferometric data of binary systems| Format | Member Price | Non-Member Price |
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Paper Abstract
Observing late type stars with an interferometer is rather easy" because of their brightness in the near-infrared and their extended atmosphere. On the other hand the interpretation of interferometric observations is very tricky, especially when it comes to asymmetric structures detected via phase measurements. Our team developed dedicated 2D Roche lobe models to interpret observations of binary candidates. The models are generated through a software that simulates binary systems in a realistic way, using a Roche representation of the stellar surfaces and the MARCS stellar atmosphere models. In this contribution we present the method and show examples of synthetic interferometric data.
Paper Details
Date Published: 24 July 2014
PDF: 5 pages
Proc. SPIE 9146, Optical and Infrared Interferometry IV, 914633 (24 July 2014); doi: 10.1117/12.2057062
Published in SPIE Proceedings Vol. 9146:
Optical and Infrared Interferometry IV
Jayadev K. Rajagopal; Michelle J. Creech-Eakman; Fabien Malbet, Editor(s)
PDF: 5 pages
Proc. SPIE 9146, Optical and Infrared Interferometry IV, 914633 (24 July 2014); doi: 10.1117/12.2057062
Show Author Affiliations
Claudia Paladini, Univ. Libre de Bruxelles (Belgium)
Alain Jorissen, Univ. Libre de Bruxelles (Belgium)
Christos Siopis, Univ. Libre de Bruxelles (Belgium)
Alain Jorissen, Univ. Libre de Bruxelles (Belgium)
Christos Siopis, Univ. Libre de Bruxelles (Belgium)
Gilles Sadowski, Univ. Libre de Bruxelles (Belgium)
Denis Shulyak, Georg-August-Univ. Göttingen (Germany)
Gianluca Li Causi, INAF - Osservatorio Astronomico di Roma (Italy)
Denis Shulyak, Georg-August-Univ. Göttingen (Germany)
Gianluca Li Causi, INAF - Osservatorio Astronomico di Roma (Italy)
Published in SPIE Proceedings Vol. 9146:
Optical and Infrared Interferometry IV
Jayadev K. Rajagopal; Michelle J. Creech-Eakman; Fabien Malbet, Editor(s)
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