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Constraints on accretion in ultraluminous X-ray sources from Spitzer IRS observations of NGC 4485/4490 : infrared diagnostic diagrams.

Vázquez, G.A. and Hornschemeier, A.E. and Colbert, E. and Roberts, T.P. and Ward, M.J. and Malhotra, S. (2007) 'Constraints on accretion in ultraluminous X-ray sources from Spitzer IRS observations of NGC 4485/4490 : infrared diagnostic diagrams.', Astrophysical journal letters., 658 (1). L21-L24.

Abstract

Constraining the astrophysical nature of ultraluminous X-ray (ULX) sources, which have X-ray luminosities exceeding 1039 ergs s1, has been elusive due to the optical faintness of any counterparts. With high spectral resolution observations in the ∼10–30 mm wavelength range we have conducted an experiment to study six ULX sources in the NGC 4485/4490 galaxy pair. We have found that five of the six ULXs, based on mid-infrared spectral diagnostics, show the characteristic higher ionization features that are found in AGNs. The sixth source, ULX-1, is consistent with being a supernova remnant. The chief infrared spectral diagnostics used are the ratios of [S iii]/[Si ii] versus [Ne iii]/[Ne ii]. In two instances fits to the continuum and polycyclic aromatic hydrocarbon (PAH) features also indicate higher dust temperatures, which are characteristic of accreting sources. Overall, however, we find that the continuum is dominated by stellar processes, and the best diagnostic features are the emission lines. High spectral resolution studies in the mid-infrared thus appear to show great promise for determining the astrophysical nature of ULXs.

Item Type:Article
Keywords:Galaxies, Individual (NGC 4485, NGC 4490, Antennae galaxies, NGC-4038/4039, Mass black-holes, Nearby galaxies, Space telescope, Star-formation, Emission, Spectrograph, Nuclear, Objects, Gas.
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Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1086/513423
Publisher statement:© 2007. The American Astronomical Society. All rights reserved.
Date accepted:No date available
Date deposited:21 February 2014
Date of first online publication:March 2007
Date first made open access:No date available

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