Please use this identifier to cite or link to this item:
http://hdl.handle.net/2307/393
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Risaliti, G. | - |
dc.contributor.author | Braito, V. | - |
dc.contributor.author | Laparola, V. | - |
dc.contributor.author | Bianchi, Stefano | - |
dc.contributor.author | Elvis, M. | - |
dc.contributor.author | Fabbiano, G. | - |
dc.contributor.author | Maiolino, R. | - |
dc.contributor.author | Matt, Giorgio | - |
dc.contributor.author | Reeves, J. | - |
dc.contributor.author | Salvati, M. | - |
dc.contributor.author | Wang, J. | - |
dc.date.accessioned | 2010-08-02T13:01:51Z | - |
dc.date.available | 2010-08-02T13:01:51Z | - |
dc.date.issued | 2009-11 | - |
dc.identifier.uri | http://hdl.handle.net/2307/393 | - |
dc.description.abstract | We present a new Suzaku observation of the obscured active galacticnucleus in NGC 1365, revealing an unexpected excess of X-rays above 20keV of at least a factor similar to 2 with respect to the extrapolationof the best-fitting 3-10 keV model. Additional Swift-BAT andIntegral-IBIS observations show that the 20-100 keV is concentratedwithin similar to 1.5 arcmin from the center of the galaxy, and is notsignificantly variable on timescales from days to years. A comparisonof this component with the 3-10 keV emission, which is characterized bya rapidly variable absorption, suggests a complex structure of thecircumnuclear medium, consisting of at least two distinct componentswith rather different physical properties, one of which covers >80% ofthe source with a column density N-H similar to 3-4x10(24) cm(-2). Analternative explanation is the presence of a double active nucleus inthe center of NGC 1365. | en |
dc.language.iso | en | en |
dc.publisher | IOP Publishing LTD | en |
dc.relation.ispartof | Astrophysical Journal Letters | en |
dc.subject | ACTIVE GALACTIC NUCLEUS | en |
dc.subject | HARD X-RAYS | en |
dc.subject | CHANDRA | en |
dc.subject | TRANSMISSION | en |
dc.subject | DISCOVERY | en |
dc.subject | GALAXY | en |
dc.subject | AGN | en |
dc.title | A strong excess in the 20-100 kev emission of ngc 1365 | en |
dc.type | Article | en |
dc.subject.miur | Settori Disciplinari MIUR::Scienze fisiche::ASTRONOMIA E ASTROFISICA | en |
dc.subject.miur | Scienze fisiche | - |
dc.subject.isicrui | Categorie ISI-CRUI::Scienze fisiche::Physics | en |
dc.subject.isicrui | Scienze fisiche | - |
dc.subject.anagraferoma3 | Scienze fisiche | en |
dc.relation.volumenumber | 705 | en |
dc.relation.pagenumber | L1–L5 | en |
dc.identifier.doi | 10.1088/0004-637X/705/1/L1 | - |
dc.relation.issuenumber | 1 | en |
dc.description.romatrecurrent | Dipartimento di Fisica 'Edoardo Amaldi' | * |
item.languageiso639-1 | other | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | restricted | - |
Appears in Collections: | A - Articolo su rivista X_Dipartimento di Fisica 'Edoardo Amaldi' |
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File | Description | Size | Format | Existing users please Login |
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astrongexcess.pdf | 482.65 kB | Adobe PDF | Request a copy |
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