| Autor: |
Copperwheat, Chris, Cropper, Mark, Soria, Roberto, Wu, Kinwah |
| Zdroj: |
Proceedings of the International Astronomical Union; 08/03/2005, Vol. 1 Issue S230, p300-301, 2p |
| Abstrakt: |
We detail a model we have created to describe the optical emission from a ULX in terms of an irradiated companion star and disk. We apply this model to optical observations of ULX X-7 in NGC 4559. We revise the parameters of the companion star in this system to be older, less massive and of a later spectral type than previously reported. We find the black hole to be of a few hundred solar masses at most. [ABSTRACT FROM PUBLISHER] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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