The Nature of the UV/Optical Emission of the Ultraluminous X-Ray Source in Holmberg II

Tao, Lian; Kaaret, Philip; Feng, Hua; Grisé, Fabien
Bibliographical reference

The Astrophysical Journal, Volume 750, Issue 2, article id. 110 (2012).

Advertised on:
5
2012
Number of authors
4
IAC number of authors
0
Citations
28
Refereed citations
27
Description
We report on UV and X-ray spectroscopy and broadband optical observations of the ultraluminous X-ray source in Holmberg II. Fitting various stellar spectral models to the combined, non-simultaneous data set, we find that normal metallicity stellar spectra are ruled out by the data, while low-metallicity, Z = 0.1 Z &sun;, late O-star spectra provide marginally acceptable fits, if we allow for the fact that X-ray ionization from the compact object may reduce or eliminate UV absorption/emission lines from the stellar wind. By contrast, an irradiated disk model fits both UV and optical data with χ2/dof = 175.9/178, and matches the nebular extinction with a reddening of E(B - V) = 0.05+0.05 - 0.04. These results suggest that the UV/optical flux of Holmberg II X-1 may be dominated by X-ray irradiated disk emission.