X-ray emission lines in ULIRGs

Hagai Netzer*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review


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

Original languageEnglish
Pages (from-to)163-168
Number of pages6
JournalAstrophysics and Space Science
Issue number1-2
StatePublished - 1999


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