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Remeis Sternwarte

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Exploring the case for hard-X-ray beaming in NGC 6946 X-1

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By James A, Remeis Sternwarte, Astronomia e astrofisica
| Oxford Academic Verified
Ultraluminous X-ray sources (ULXs; see the reviews of Roberts 2007; Kaaret, Feng & Roberts 2017; King, Lasota & Middleton 2023) are known to contain stellar remnants in the form of neutron stars and probably stellar mass black holes (although the relative number remains unknown, see e.g. Middleton & King 2016; King & Lasota 2020).
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