Pietsch W, Haberl F, Sasaki M, Gaetz TJ, Plucinsky PP, Ghavamian P, Long KS, Pannuti T (2006)
Publication Status: Published
Publication Type: Journal article
Publication year: 2006
Publisher: UNIV CHICAGO PRESS
Book Volume: 646
Pages Range: 420-428
Journal Issue: 1
The first observations conducted as part of the Chandra ACIS survey of M33 (ChASeM33) sampled the eclipsing X-ray binary M33 X-7 over a large part of the 3.45 day orbital period and have resolved eclipse ingress and egress for the first time. The occurrence of the X-ray eclipse allows us to determine an improved ephemeris of mid-eclipse and binary period as HJD (2; 453; 639.119 +/- 0.005) +/- N(3.453014 +/- 0.000020) and constrain the eclipse half-angle to 26 degrees.5 +/- 1 degrees.1. There are indications for a shortening of the orbital period. The X-ray spectrum is best described by a disk blackbody spectrum typical for black hole X-ray binaries in the Galaxy. We find a flat power density spectrum, and no significant regular pulsations were found in the frequency range of 10(-4) to 0.15 Hz. HST WFPC2 images resolve the optical counterpart, which can be identified as an O6 III star with the help of extinction and color corrections derived from the X-ray absorption. Based on the optical light curve, the mass of the compact object in the system most likely exceeds 9 M-circle dot. This mass, the shape of the X-ray spectrum, and the short-term X-ray time variability identify M33 X-7 as the first eclipsing black hole high-mass X-ray binary.
APA:
Pietsch, W., Haberl, F., Sasaki, M., Gaetz, T.J., Plucinsky, P.P., Ghavamian, P.,... Pannuti, T. (2006). M33 X-7: ChASeM33 reveals the first eclipsing black hole X-ray binary. Astrophysical Journal, 646(1), 420-428.
MLA:
Pietsch, Wolfgang, et al. "M33 X-7: ChASeM33 reveals the first eclipsing black hole X-ray binary." Astrophysical Journal 646.1 (2006): 420-428.
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