The Modulated Emission of the Ultraluminous X-Ray Source in NGC 3379

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Summary

It is argued that the results establish this source as a ULX binary in NGC 3379 as a soft transient, given the old stellar population of this galaxy, and the current ‘‘on’’ phase has lasted � 10 yr.

Type
preprint
Published
2006-10-20
Cited by
15
References
54
Access
Open access

Keywords

Physics, Astrophysics, Flux (metallurgy), Galaxy, Orbital period

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