DISK-DOMINATED STATES OF 4U 1957+11: CHANDRA, XMM-NEWTON, AND RXTE OBSERVATIONS OF OSTENSIBLY THE MOST RAPIDLY SPINNING GALACTIC BLACK HOLE

Nowak MA, Juett A, Homan J, Yao Y, Wilms J, Schulz NS, Canizares CR (2008)

Publication Status: Published

Publication Type: Journal article

Publication year: 2008

Journal

Astrophysical Journal American Astronomical Society

Publisher: IOP PUBLISHING LTD

Book Volume: 689

Pages Range: 1199-1214

Journal Issue: 2

Abstract

We present simultaneous Chandra High-Energy Transmission Gratings (HETG) and Rossi X-ray Timing Explorer (RXTE) observations of a "soft state'' of the black hole candidate 4U 1957+11. These spectra, having limited hard X-ray excess, are an excellent test of disk atmosphere models that include effects of black hole spin. The HETG data show, by modeling the broadband continuum and direct fitting of absorption edges, that the disk spectrum is only very mildly absorbed, with N-H = (1-2) x 10(21) cm(-2). These data additionally reveal lambda lambda 13.449 Ne IX absorption consistent with the warm/ hot phase of the interstellar medium. The fitted disk model implies an inclined disk around a low-mass black hole rotating with normalized spin a* approximate to 1. We show, however, that pure Schwarzschild models describe the data extremely well, albeit with large disk atmosphere "color-correction'' factors. Standard correction factors can be attained if one incorporates mild Comptonization. We find that the Chandra observations do not uniquely determine spin, even with this otherwise extremely well-measured, nearly pure disk spectrum. XMM-Newton RXTE observations, taken only six weeks later, are equally unconstraining. This lack of constraint is partly driven by the unknown mass and distance of 4U 1957+ 11; however, it is also driven by the limited Chandra and XMM-Newton bandpasses. We therefore present a series of 48 RXTE observations taken at different brightness/ hardness levels. These data prefer a spin of a* approximate to 1, even when including a mild Comptonization component; however, they also show evolution of the color-correction factors. If the rapid-spin models with standard correction factors are to be believed, then the RXTE observations predict that 4U 1957+ 11 can range from a 3 M-circle dot black hole at 10 kpc with a* approximate to 0: 83 to a 16 M-circle dot black hole at 22 kpc with

Authors with CRIS profile

Jörn Wilms Professur für Astronomie und Astrophysik

Involved external institutions

Massachusetts Institute of Technology (MIT) US United States (USA) (US) University of Virginia (UVA) US United States (USA) (US)

How to cite

APA:

Nowak, M.A., Juett, A., Homan, J., Yao, Y., Wilms, J., Schulz, N.S., & Canizares, C.R. (2008). DISK-DOMINATED STATES OF 4U 1957+11: CHANDRA, XMM-NEWTON, AND RXTE OBSERVATIONS OF OSTENSIBLY THE MOST RAPIDLY SPINNING GALACTIC BLACK HOLE. Astrophysical Journal, 689(2), 1199-1214.

MLA:

Nowak, Michael A., et al. "DISK-DOMINATED STATES OF 4U 1957+11: CHANDRA, XMM-NEWTON, AND RXTE OBSERVATIONS OF OSTENSIBLY THE MOST RAPIDLY SPINNING GALACTIC BLACK HOLE." Astrophysical Journal 689.2 (2008): 1199-1214.

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