Benvenuti nell'Anagrafe della Ricerca d'Ateneo
La valutazione delle attività di ricerca che si svolgono nelle università ha assunto un'importanza rilevante sia per l'intero sistema universitario sia all'interno di ogni singolo ateneo. Roma Tre si è quindi dotata di idonei strumenti informativi in grado di supportare al meglio le azioni di monitoraggio e di valutazione delle attività di ricerca svolte nei propri dipartimentied ha realizzato una Anagrafe della Ricerca di Ateneo.
EnglishWe analyse Chandra, XMM-Newton and Hubble Space Telescope (HST) data of the double-nucleus Ultraluminous Infrared Galaxy (ULIRG), Mrk 463. The Chandra detection of two luminous (L2-10 keV = 1.5 x 10(43) and 3.8 x 10(42) erg cm(-2) s(-1)), unresolved nuclei in Mrk 463 indicates that this galaxy hosts a binary active galactic nucleus (AGN), with a projected separation of similar or equal to 3.8 kpc (3.83 +/- 0.01 arcsec). While the East nucleus was already known to be a type 2 Seyfert (and this is further confirmed by our Chandra detection of a neutral iron line), this is the first unambiguous evidence in favour of the AGN nature of the West nucleus. Mrk 463 is therefore the clearest case so far for a binary AGN, after NGC 6240.
Bianchi S, Chiaberge M, Piconcelli E, Guainazzi M, & Matt G (2008). Chandra unveils a binary active galactic nucleus in Mrk 463 RID B-4804-2010. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 386(1), 105-110.
| Titolo: | Chandra unveils a binary active galactic nucleus in Mrk 463 RID B-4804-2010 | |
| Autori: | ||
| Data di pubblicazione: | 2008 | |
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| Citazione: | Bianchi S, Chiaberge M, Piconcelli E, Guainazzi M, & Matt G (2008). Chandra unveils a binary active galactic nucleus in Mrk 463 RID B-4804-2010. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 386(1), 105-110. | |
| Abstract: | We analyse Chandra, XMM-Newton and Hubble Space Telescope (HST) data of the double-nucleus Ultraluminous Infrared Galaxy (ULIRG), Mrk 463. The Chandra detection of two luminous (L2-10 keV = 1.5 x 10(43) and 3.8 x 10(42) erg cm(-2) s(-1)), unresolved nuclei in Mrk 463 indicates that this galaxy hosts a binary active galactic nucleus (AGN), with a projected separation of similar or equal to 3.8 kpc (3.83 +/- 0.01 arcsec). While the East nucleus was already known to be a type 2 Seyfert (and this is further confirmed by our Chandra detection of a neutral iron line), this is the first unambiguous evidence in favour of the AGN nature of the West nucleus. Mrk 463 is therefore the clearest case so far for a binary AGN, after NGC 6240. | |
| Handle: | http://hdl.handle.net/11590/132527 | |
| Appare nelle tipologie: | 1.1 Articolo in rivista |
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