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X-ray Emission Lines in ULIRGs

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Abstract

Fits to ASCA data allow the first classification of ULIRG spectra into starburst dominated and AGN dominated. New calculations presented here demonstratethe expected improvementin such analysis, in the near future, when three advanced X-ray missions willenable proper measurements of X-ray lines in such objects.

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Netzer, H. X-ray Emission Lines in ULIRGs. Astrophysics and Space Science 266, 163–168 (1999). https://doi.org/10.1023/A:1002666102185

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  • DOI: https://doi.org/10.1023/A:1002666102185

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