HOT THERMAL X-RAY EMISSION FROM THE Be STAR HD 119682

We present an analysis of a series of four consecutive Chandra high-resolution transmission gratings observations, amounting to a total of 150 ks, of the Be X-ray source HD 119682 (=1WGA J1346.5-6255), a member of the new class of γ Cas analogs. The Chandra light curve shows significant brightness v...

Full description

Bibliographic Details
Main Authors: Torrejón, J. M. (Author), Testa, P. (Author), Rodes, J. J. (Author), Nowak, Michael A. (Contributor), Schulz, Norbert S. (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2015-01-29T18:56:38Z.
Subjects:
Online Access:Get fulltext