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.
Similar content being viewed by others
References
Nakagawa, T., 1999 (this volume)
Netzer, H., (1996) X-ray Lines in Active Galactic Nuclei and Photoionized Gases, ApJ, Vol. no. 483, pp. 781-796
Netzer, H., and Turner, T.J., (1997) Soft X-ray Lines and Gas Composition in NGC 1068, ApJ, Vol. no. 488, pp. 694-701
Netzer, H., Turner, T.G, and George, I.M., (1998) The Soft X-ray Spectrum of Scattering Dominated Active Galactic Nuclei, ApJ, Vol. no. 504, pp. 680-692
Ptak, A., Serlemitsos, P., Yaqoob, T., and Mushotzky, R.F., (1997) The Complex X-ray Spectra of M82 and NGC 253, AJ, Vol. no. 113, pp. 1286-1295
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Netzer, H. X-ray Emission Lines in ULIRGs. Astrophysics and Space Science 266, 163–168 (1999). https://doi.org/10.1023/A:1002666102185
Issue Date:
DOI: https://doi.org/10.1023/A:1002666102185