Mostrar el registro sencillo

dc.contributor.authorFeltre, A.
dc.contributor.authorHatziminaoglou, Evanthia
dc.contributor.authorHernán Caballero, Antonio
dc.contributor.authorFritz, J.
dc.contributor.authorFranceschini, Alberto
dc.contributor.authorBock, Jamie
dc.contributor.authorCooray, Asantha R.
dc.contributor.authorFarrah, Duncan
dc.contributor.authorGonzález Solares, Eduardo A.
dc.contributor.authorIbar, Edo
dc.contributor.authorIsaak, K. G.
dc.contributor.authorLo Faro, B.
dc.contributor.authorMarchetti, L.
dc.contributor.authorOliver, Seb
dc.contributor.authorPage, Mathew J.
dc.contributor.authorRigopoulou, Dimitra
dc.contributor.authorRoseboom, I. G.
dc.contributor.authorSymeonidis, M.
dc.contributor.authorVaccari, Mattia
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2014-06-12T08:08:06Z
dc.date.available2014-06-12T08:08:06Z
dc.date.issued2013-09
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttp://hdl.handle.net/10902/4815
dc.description.abstractIn this work, we explore the impact of the presence of an active galactic nucleus (AGN) on the mid- and far-infrared (IR) properties of galaxies as well as the effects of simultaneous AGN and starburst activity in the same galaxies. To do this, we apply a multicomponent, multiband spectral synthesis technique to a sample of 250 μm selected galaxies of the Herschel Multi-tiered Extragalactic Survey (HerMES), with Infrared Spectrograph (IRS) spectra available for all galaxies. Our results confirm that the inclusion of the IRS spectra plays a crucial role in the spectral analysis of galaxies with an AGN component improving the selection of the best-fitting hot dust (torus) model. We find a correlation between the obscured star formation rate, SFRIR, derived from the IR luminosity of the starburst component, and SFRPAH, derived from the luminosity of the PAH features, LPAH, with SFRFIR taking higher values than SFRPAH. The correlation is different for AGN- and starburst-dominated objects. The ratio of LPAH to that of the starburst component, LPAH/LSB, is almost constant for AGN-dominated objects but decreases with increasing LSB for starburst-dominated objects. SFRFIR increases with the accretion luminosity, Lacc, with the increase less prominent for the very brightest, unobscured AGN-dominated sources. We find no correlation between the masses of the hot (AGN-heated) and cold (starburst-heated) dust components. We interpret this as a non-constant fraction of gas driven by the gravitational effects to the AGN while the starburst is ongoing. We also find no evidence of the AGN affecting the temperature of the cold dust component, though this conclusion is mostly based on objects with a non-dominant AGN component. We conclude that our findings do not provide evidence that the presence of AGN affects the star formation process in the host galaxy, but rather that the two phenomena occur simultaneously over a wide range of luminosities.es_ES
dc.format.extent12 p.es_ES
dc.language.isoenges_ES
dc.publisherOxford University Presses_ES
dc.publisherRoyal Astronomical Societyes_ES
dc.rights© 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society*
dc.sourceMonthly Notices of the Royal Astronomical Society, vol. 434, iss.3, Pp.2426-2437 (2013)es_ES
dc.subject.otherGalaxies: activees_ES
dc.subject.otherGalaxies: starburstes_ES
dc.subject.otherGalaxies: star formationes_ES
dc.subject.otherInfrared: galaxieses_ES
dc.titleThe roles of star formation and AGN activity of IRS sources in the HerMES fieldses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttp://dx.doi.org/10.1093/mnras/stt1177es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1093/mnras/stt1177
dc.type.versionpublishedVersiones_ES


Ficheros en el ítem

Thumbnail

Este ítem aparece en la(s) siguiente(s) colección(ones)

Mostrar el registro sencillo