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Paper published in a journal (Scientific congresses and symposiums)
Apsidal motion in the massive binary HD 152248
Rosu, Sophie; Rauw, Grégor; Gosset, Eric et al.
2020In Contributions of the Astronomical Observatory Skalnaté Pleso, 50 (2), p. 624-626
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Keywords :
stars: early-type; stars: individual: HD 152248; stars: massive; binaries: spectroscopic; binaries: eclipsing
Abstract :
[en] The eccentric massive binary HD 152248, hosting two very similar O7.5 III(f) stars, is the most emblematic eclipsing O-star binary in the very young and rich open cluster NGC 6231. Measuring the rate of apsidal motion in such a binary system gives insight into the internal structure and evolutionary state of the stars composing it.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Rosu, Sophie  ;  Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Rauw, Grégor  ;  Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Gosset, Eric ;  Université de Liège - ULiège > Groupe d'astrophysique des hautes énergies (GAPHE)
Manfroid, Jean  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO)
Royer, Pierre
Language :
English
Title :
Apsidal motion in the massive binary HD 152248
Publication date :
March 2020
Event name :
Universe of Binaries, Binaries in the Universe
Event place :
Telc, Czechia
Event date :
Du 7 septembre 2019 au 11 septembre 2019
Audience :
International
Journal title :
Contributions of the Astronomical Observatory Skalnaté Pleso
ISSN :
1335-1842
eISSN :
1336-0337
Publisher :
Astronomicky Ustav SAV, Slovakia
Volume :
50
Issue :
2
Pages :
624-626
Peer reviewed :
Peer Reviewed verified by ORBi
Funders :
F.R.S.-FNRS - Fonds de la Recherche Scientifique
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since 07 April 2020

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