Survey of supersoft and quasisoft X-ray sources in the Magellanic Clouds with XMM-Newton and Chandra
Supersoft and quasisoft X-ray sources are collectively known as Very Soft X-ray Sources (VSSs) characterized by their considerably lower effective temperatures than normal X-ray emitting objects and the lack of significant emission above 1 keV, with measured temperatures ranging from about tens to l...
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| Language: | English |
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The University of Hong Kong (Pokfulam, Hong Kong)
2013
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| Online Access: | http://hdl.handle.net/10722/193077 |