A mass of less than 15 solar masses for the black hole in an ultraluminous X-ray source
Most ultraluminous X-ray sources have a typical set of properties not seen in Galactic stellar-mass black holes. They have luminosities of more than 3 × 10 39 ergs per second, unusually soft X-ray components (with a typical temperature of less than about 0.3 kiloelectronvolts) and a characteristic d...
| Main Authors: | Motch, C., Pakull, M., Soria, Roberto, Grisé, F., Pietrzynski, G. |
|---|---|
| Format: | Journal Article |
| Published: |
Nature Publishing Group
2014
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| Online Access: | http://hdl.handle.net/20.500.11937/8687 |
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