Reference : The mysterious high-latitude O-star HD 93521: new results from XMM-Newton observations
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/97147
The mysterious high-latitude O-star HD 93521: new results from XMM-Newton observations
English
Rauw, Grégor mailto [Institut d'Astrophysique & Géophysique, University of Liège, Allée du 6 Août 17, B-4000, Liège, Belgium]
Morel, Thierry mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Groupe d'astrophysique des hautes énergies (GAPHE)]
1-Jul-2011
Active OB stars: structure, evolution, mass loss and critical limits
[en] Proceedings IAU Symposium no. 272
Neiner, Coralie
Wade, G.
Meynet, G.
Peters, G.
612-613
No
No
International
[en] stars: early-type ; stars: individual (HD 93521) ; X-rays: stars
[en] The O9.5 Vp star HD 93521 is a well known non-radial pulsator located at a high Galactic latitude. The nature (Population I vs. II) of this star has been the subject of controversy for many years. We report on an XMM-Newton observation of the star that sheds new light on its nature.
http://hdl.handle.net/2268/97147
10.1017/S1743921311011550
http://adsabs.harvard.edu/abs/2011IAUS..272..612R

File(s) associated to this reference

Fulltext file(s):

FileCommentaryVersionSizeAccess
Restricted access
S1743921311011550a.pdfPublisher postprint152.95 kBRequest copy

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.