A 33 hour period for the Wolf-Rayet/black hole X-ray binary candidate NGC 300 X-1

Details A 33 hour period for the Wolf-Rayet/black hole X-ray binary candidate NGC 300 X-1 A 33 hour period for the Wolf-Rayet/black hole X-ray binary candidate NGC 300 X-1

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel..974....1c&link_type=abstract

The Astronomer's Telegram, #974

Astronomy and Astrophysics

Astronomy

X-Ray, Binaries, Black Holes

Scientific paper

NGC 300 X-1 is the second extragalactic candidate, after IC 10 X-1, for the rare class of Wolf-Rayet/compact object X-ray binary system (Carpano et al. 2007, A&A, 461,9L) uniquely exemplified in the Galaxy by Cyg X-3.
From a theoretical point of view, these systems should have orbital periods up to several tens of hours (Ergma & Yungelson, 1998, A&A, 333, 151; Lommen et al., 2005, A&A, 443, 231L).

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