Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/25163
Title: A variable ultraluminous supersoft X-ray source in ''the antennae'': Stellar-mass black hole or white dwarf?
Authors: Fabbiano, G.
King, A. R.
Zezas, A.
Ponman, T. J.
Rots, A.
Schweizer, F.
First Published: 10-Jul-2003
Publisher: UNIV CHICAGO PRESS
Citation: Astrophysical Journal, 2003, 591 (2), pp. 843-849
Abstract: The Chandra monitoring observations of "The Antennae" (NGC 4038/4039) have led to the discovery of a variable, luminous, supersoft source (SSS). This source is detected only at energies below 2 keV and, in 2002 May, reached count rates comparable to those of the nine ultraluminous X-ray sources (ULXs) detected in these galaxies. Spectral fits of the SSS data give acceptable results only for a ~90-100 eV blackbody spectrum with an intrinsic absorption column of NH ~ (2-3) × 1021 cm-2. For a distance of 19 Mpc, the best-fit observed luminosity increases from 1.7 × 1038 ergs s-1 in 1999 December to 8.0 × 1038 ergs s-1 in 2002 May. The intrinsic, absorption-corrected, best-fit luminosity reaches 1.4 × 1040 ergs s-1 in 2002 May. The assumption of unbeamed emission would suggest a black hole of gsim100 M☉. However, if the emission is blackbody at all times, as suggested by the steep soft spectrum, the radiating area would have to vary by a factor of ~103, inconsistent with gravitational energy release from within a few Schwarzschild radii of a black hole. Viable explanations for the observed properties of the SSS are provided by anisotropic emission from either an accreting nuclear-burning white dwarf or an accreting stellar-mass black hole.
DOI Link: 10.1086/375441
ISSN: 0004-637X
Links: http://hdl.handle.net/2381/25163
http://iopscience.iop.org/article/10.1086/375441/meta
Type: Journal Article
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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