Revisiting the ultraluminous supersoft source in M 101: An optically thick outflow model

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Revisiting the ultraluminous supersoft source in M 101: An optically thick outflow model

The M 101 galaxy contains the best-known example of an ultraluminous supersoft source (ULS), dominated by a thermal component at kT ≈ 0.1 keV. The origin of the thermal component and the relation between ULSs and standard (broad-band spectrum) ultraluminous X-ray sources are still controversial. We...

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Bibliographic Details
Main Authors:	Soria, Roberto, Kong, A.
Format:	Journal Article
Published:	Oxford University Press 2016
Online Access:	http://hdl.handle.net/20.500.11937/44333

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