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dc.contributor.authorNazé, Yaël
dc.contributor.authorWade, Gregg A.
dc.contributor.authorPetit, Véronique
dc.date.accessioned2014-11-14T15:25:51Z
dc.date.available2014-11-14T15:25:51Z
dc.date.issued2014-09-25
dc.identifier.citationNazé, Y., Wade, G. A., & Petit, V. (2014). Modulated X-ray emission of the magnetic O8.5V-star Tr16-22. Astronomy and Astrophysics, 569en_US
dc.identifier.urihttp://hdl.handle.net/11141/406
dc.description.abstractUsing an extensive X-ray dataset, we analyzed the X-ray emission of the massive O-star Tr16-22, which was recently found to be magnetic. Its bright X-ray emission is found to be modulated with a 54d period. This timescale should represent the rotational timescale of the star, as it does for other magnetic massive stars. In parallel, new spectropolarimetric data confirm the published magnetic detection.en_US
dc.language.isoen_USen_US
dc.rightsThis published article is available in accordance with the publisher's policy. It may be subject to U.S. Copyright Law.en_US
dc.rights.urihttp://www.aanda.org/index.php?option=com_content&view=article&id=863&Itemid=295en_US
dc.titleModulated X-ray emission of the magnetic O8.5V-star Tr16-22en_US
dc.typeArticleen_US
dc.identifier.doi10.1051/0004-6361/201424416


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