The optical counterpart of the superluminal source GRO J1655 – 40
The optical counterpart of the superluminal source GRO J1655 – 40
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London: Nature Publishing Group UK
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English
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London: Nature Publishing Group UK
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THE accretion of gas from a companion star onto a compact object, such as a neutron star or black hole, can release large amounts of energy. Episodic accretion is generally thought to explain transient X-ray emission, such as that associated with the recently discovered
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Galactic superluminal source GRO J1655 – 40, and to be connected with t...
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Full title
The optical counterpart of the superluminal source GRO J1655 – 40
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TN_cdi_proquest_miscellaneous_743512752
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_743512752
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ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/374701a0
