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