X-Ray Outflows and Super-Eddington Accretion in the Ultraluminous X-Ray Source Holmberg IX X-1
Abstract
Studies of X-ray continuum emission and flux variability have not conclusively revealed the nature of ultraluminous X-ray sources (ULXs) at the high-luminosity end of the distribution (those with L_X ≥ 10^(40) erg s^(–1)). These are of particular interest because the luminosity requires either super-Eddington accretion onto a black hole of mass ~10 M☉ or more standard accretion onto an intermediate-mass black hole. Super-Eddington accretion models predict strong outflowing winds, making atomic absorption lines a key diagnostic of the nature of extreme ULXs. To search for such features, we have undertaken a long, 500 ks observing campaign on Holmberg IX X-1 with Suzaku. This is the most sensitive data set in the iron K bandpass for a bright, isolated ULX to date, yet we find no statistically significant atomic features in either emission or absorption; any undetected narrow features must have equivalent widths less than 15-20 eV at 99% confidence. These limits are far below the ≳150 eV lines expected if observed trends between mass inflow and outflow rates extend into the super-Eddington regime and in fact rule out the line strengths observed from disk winds in a variety of sub-Eddington black holes. We therefore cannot be viewing the central regions of Holmberg IX X-1 through any substantial column of material, ruling out models of spherical super-Eddington accretion. If Holmberg IX X-1 is a super-Eddington source, any associated outflow must have an anisotropic geometry. Finally, the lack of iron emission suggests that the stellar companion cannot be launching a strong wind and that Holmberg IX X-1 must primarily accrete via Roche-lobe overflow.
Additional Information
© 2013 The American Astronomical Society. Received 2013 April 27; accepted 2013 June 8; published 2013 July 26. The authors thank the reviewer for helpful comments. This research has made use of data obtained from the Suzaku observatory, a collaborative mission between the space agencies of Japan (JAXA) and the USA (NASA).Attached Files
Published - 2041-8205_773_1_L9.pdf
Submitted - 1306.2317v1.pdf
Files
Name | Size | Download all |
---|---|---|
md5:819a67366194dd7ce67f52d4ea2403c4
|
499.1 kB | Preview Download |
md5:e10e9bc29c79eb08fe6804030ca09a95
|
196.8 kB | Preview Download |
Additional details
- Eprint ID
- 41161
- Resolver ID
- CaltechAUTHORS:20130909-090748501
- Created
-
2013-09-17Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory