The X-ray properties of magnetic massive stars

Yaël Nazé, Véronique Petit, Melanie Rinbrand, David Cohen, Stan Owocki, Asif Ud-Doula, Gregg Wade

Research output: Contribution to journalArticle

Abstract

Early-type stars are well-known to be sources of soft X-rays. However, this high-energy emission can be supplemented by bright and hard X-rays when magnetically confined winds are present. In an attempt to clarify the systematics of the observed X-ray properties of this phenomenon, a large series of Chandra and XMM observations was analyzed, over 100 exposures of 60% of the known magnetic massive stars listed recently by Petit et al. (2013). It is found that the X-ray luminosity is strongly correlated with mass-loss rate, in agreement with predictions of magnetically confined wind models, though the predictions of higher temperature are not always verified. We also investigated the behaviour of other X-ray properties (absorption, variability), yielding additional constraints on models. This work not only advances our knowledge of the X-ray emission of massive stars, but also suggests new observational and theoretical avenues to further explore magnetically confined winds.

Original languageEnglish (US)
Pages (from-to)437-442
Number of pages6
JournalProceedings of the International Astronomical Union
Volume9
DOIs
StatePublished - Jan 1 2014

All Science Journal Classification (ASJC) codes

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'The X-ray properties of magnetic massive stars'. Together they form a unique fingerprint.

Cite this