Probing the Hot X-Ray Corona around the Massive Spiral Galaxy, NGC 6753, Using Deep
X-ray emitting gaseous coronae around massive galaxies are a basic prediction of galaxy formation models. Although the coronae around spiral galaxies offer a fundamental test of these models, observational constraints on their characteristics are still scarce. While the presence of extended hot coro...
| Main Authors: | , , , , , , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
American Astronomical Society,
2018-08-28T13:10:59Z.
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| Subjects: | |
| Online Access: | Get fulltext |