Eales, Stephen Anthony ![]() |
Official URL: http://dx.doi.org/10.1086/165889
Abstract
The Einstein X-ray data for the two luminous infrared galaxies, Arp 220 and Markarian 231 have been analyzed. There is an X-ray source about 1 arcmin from the position of Arp 220 that is probably associated with it. Mrk 231 was not detected. The size of the source and its soft X-ray spectrum implies that the bulk of the X-ray emission from Arp 220 cannot be coming from the obscured active nucleus at the galaxy's center. The absence of strong X-ray emission from the active nuclei in Arp 220 and Mrk 231 suggests that there must be more line-of-sight absorption to the active nuclei than is inferred from many of the absorption indicators available.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Uncontrolled Keywords: | active galactic nuclei; astronomical spectroscopy; far infrared radiation; galactic structure; markarian galaxies; x ray sources; absorption spectra; emission spectra |
Publisher: | IOP Science |
ISSN: | 0004-637X |
Last Modified: | 24 Oct 2022 11:14 |
URI: | https://orca.cardiff.ac.uk/id/eprint/47425 |
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