The Elusive Active Nucleus of NGC 4945

dc.creatorMarconi, A.
dc.creatorOliva, E.
dc.creatorvan der Werf, P. P.
dc.creatorMaiolino, R.
dc.creatorSchreier, E. J.
dc.creatorMacchetto, F.
dc.creatorMoorwood, A. F. M.
dc.date2000-02-11
dc.date.accessioned2026-07-25T11:00:41Z
dc.descriptionWe present new HST NICMOS observations of NGC 4945, a starburst galaxy hosting a highly obscured active nucleus that is one of the brightest extragalactic sources at 100 keV. The HST data are complemented with ground based [FeII] line and mid--IR observations. A 100pc-scale starburst ring is detected in Pa alpha, while H_2 traces the walls of a super bubble opened by supernova-driven winds. The conically shaped cavity is particularly prominent in Pa alpha equivalent width and in the Pa alpha/H_2 ratio. Continuum images are heavily affected by dust extinction and the nucleus of the galaxy is located in a highly reddened region with an elongated, disk-like morphology. No manifestation of the active nucleus is found, neither a strong point source nor dilution in CO stellar features, which are expected tracers of AGN activity. Even if no AGN traces are detected in the near-IR, with the currently available data it is still not possible to establish whether the bolometric luminosity of the object is powered by the AGN or by the starburst: we demonstrate that the two scenarios constitute equally viable alternatives. However, the absence of any signature other than in the hard X-rays implies that, in both scenarios, the AGN is non-standard: if it dominates, it must be obscured in all directions, conversely, if the starburst dominates, the AGN must lack UV photons with respect to X-rays. An important conclusion is that powerful AGNs can be hidden even at mid-infrared wavelengths and, therefore, the nature of luminous dusty galaxies cannot be always characterized by long-wavelength data alone but must be complemented with sensitive hard X-ray observations.
dc.descriptionAccepted for publication in A&A, high quality color pictures available at http://www.arcetri.astro.it/~marconi/colpic.html
dc.identifierhttps://arxiv.org/abs/astro-ph/0002244
dc.identifierhttp://arxiv.org/abs/astro-ph/0002244
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/512
dc.subjectAstrophysics
dc.titleThe Elusive Active Nucleus of NGC 4945
dc.typetext

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