A newly discovered double-double candidate microquasar in NGC 300
We present the discovery of a powerful candidate microquasar in NGC 300, associated with the S 10 optical nebula (previously classified as a supernova remnant). Chandra images show four discrete X-ray knots aligned in the plane of the sky over a length of ≈150 pc. The X-ray emission from the knots i...
| Main Authors: | , , , , , , , , , |
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| Format: | Journal Article |
| Published: |
Oxford University Press
2019
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| Online Access: | http://purl.org/au-research/grants/arc/DE180100346 http://hdl.handle.net/20.500.11937/73670 |