... The characterization of the nuclear star forming region (its age and mass) is very difficult to achieve in AGN, due to the contamination of the nuclear stellar absorption lines by the AGN component itself. ...
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Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P7-9.pdf -- 223.0 Кб -- 27.08.2004 Похожие документы
... The characterization of the nuclear star forming region (its age and mass) is very difficult to achieve in AGN, due to the contamination of the nuclear stellar absorption lines by the AGN component itself. ...
... different types of stars or, say, QSO and AGN should be expected because of original ... One person's QSO is another's AGN or galaxy. ... been classified by the OC1 classifier as AGN and Cluster, respectively, which partly ...
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Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/P4-10.pdf -- 390.6 Кб -- 11.03.2003 Похожие документы
... A starburst-dominant galaxy could consist of 30% photodissociation region (PDR), 55% starburst (SB) and 15% Active Galactic Nucleus (AGN) SED TEMPLATES Spectral Energy Distribution (SED) template files for the three galaxy types: PDR, SB, AGN. ...
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Ссылки http://www.adass.org/adass/proceedings/adass00/reprints/P2-48.pdf -- 71.3 Кб -- 29.05.2001 Похожие документы
... different types of stars or, say, QSO and AGN should be expected because of original ... A class is rarely a clear-cut notion. One person's QSO is another's AGN or galaxy. ...
... than X-ray sources, and provides quasi-real-time data of, for instance, AGN variability and X-ray Novae through the internet ... Kawai, N., Negoro, H., Yoshida, A., Mihara, T. (Eds.), 2003, in MAXI Workshop on AGN Variability, (Seiyo Press: Tokyo) . ...