X-RAY EMISSION AND CORONA OF THE YOUNG INTERMEDIATE-MASS BINARY theta(1) Ori E
θ(1) Ori E is a young, moderate mass binary system, a rarely observed case of spectral-type G-giants of about 3 solar masses, which are still collapsing toward the main sequence, where they presumably become X-ray faint. We have obtained high-resolution X-ray spectra with Chandra and find that the s...
| Main Authors: | , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
American Astronomical Society
2010
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| Online Access: | http://hdl.handle.net/1721.1/51722 https://orcid.org/0000-0002-5769-8441 |