CHANDRA CHARACTERIZATION OF X-RAY EMISSION IN THE YOUNG F-STAR BINARY SYSTEM HD 113766

Using Chandra, we have obtained imaging X-ray spectroscopy of the 10-16 Myr old F-star binary HD 113766. We individually resolve the 1[fraction of arcsecond]4 separation binary components for the first time in the X-ray and find a total 0.3-2.0 keV luminosity of 2.2 × 10[superscript 29] erg s[supers...

Full description

Bibliographic Details
Main Authors: Lisse, C. M. (Author), Christian, D. J. (Author), Wolk, S. J. (Author), Chen, C. H. (Author), Grady, C. A. (Author), Guenther, Hans Moritz (Contributor)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-06-21T15:19:21Z.
Subjects:
Online Access:Get fulltext