Optical modulation of the new eclipsing XRB in M33

Details Optical modulation of the new eclipsing XRB in M33 Optical modulation of the new eclipsing XRB in M33

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..913....1s&link_type=abstract

The Astronomer's Telegram, #913

Astronomy and Astrophysics

Astronomy

1

Optical, Binaries

Scientific paper

The variable XMM-Newton source [PMH2004] 47 was recently identified by
Pietsch et al. (ATel #905) as an eclipsing XRB with an orbital period of
1.73245 days. Based on its position and color, Pietsch et al.
identified star #4571 of Massey et al. (2006, AJ 131, 2478) as the
optical counterpart of the X-ray source.

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