期刊
ASTROPHYSICAL JOURNAL
卷 581, 期 1, 页码 L9-L13出版社
UNIV CHICAGO PRESS
DOI: 10.1086/345925
关键词
galaxies : active; galaxies : individual (IC 694, NGC 3690); galaxies : nuclei; galaxies : starburst; X-rays : galaxies
Using a long (similar or equal to150 ks) broadband (0.1- 40 keV) BeppoSAX observation of the merging starburst system Arp 299 (=IC 694 + NGC 3690), we found the first unambiguous evidence of the presence of a deeply buried (N-H similar or equal to 2.5 x 10(24) cm(-2)) active galactic nucleus (AGN) having an intrinsic luminosity of L0.5-100 (keV) similar or equal to 1.9 x 10(43) ergs s(-1). The X- ray spectral properties of this AGN are discussed in detail, as well as the thermal component detected at soft X- ray energies, which, most likely, is associated with the starburst.
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