Chandra and Hubble Space Telescope Confirmation of the Luminous and Variable X-Ray Source IC 10 X-1 as a Possible Wolf-Rayet, Black Hole Binary

Abstract

We present a Chandra and Hubble Space Telescope study of IC 10 X-1, the most luminous X-ray binary in the starburst galaxy closest to the Milky Way. Our new hard X-ray observation of X-1 confirms that it has an average 0.5-10 keV luminosity of 1.5 × 10 38 ergs s -1 , is strongly variable (a factor of ≈2 in ##IMG## [http://ej.iop.org/icons/Entities/lesssim.gif] {lesssim} 3 ks), and is spatially coincident (within 0 ##IMG## [http://ej.iop.org/icons/Entities/farcs.gif] {farcs} 23 ± 0 ##IMG## [http://ej.iop.org/icons/Entities/farcs.gif] {farcs} 30) with the Wolf-Rayet (W-R) star [MAC92] 17A in IC 10. The spectrum of X-1 is best fitted by a power law with Γ ≈ 1.8 and a thermal plasma with kT ≈ 1.5 keV, although systematic residuals hint at further complexity. Taken together, these facts suggest that X-1 may be a black hole belonging to the rare class of W-R binaries; it is comparable in many ways to Cyg X-3. The Chandra observation also finds evidence for extended X-ray emission cospatial with the large nonthermal radio superbubble surrounding X-1.