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Extinction law variations and dust excitation in the spiral galaxy NGC 300

dc.contributor.authorRoussel, H.
dc.contributor.authorGil De Paz, Armando
dc.contributor.authorSeibert, M.
dc.contributor.authorHelou, G;, G.
dc.contributor.authorMadore, B. F.
dc.contributor.authorMartín, C.
dc.date.accessioned2023-06-20T11:09:31Z
dc.date.available2023-06-20T11:09:31Z
dc.date.issued2005-10-10
dc.description© 2005. The American Astronomical Society. All rights reserved. We thank Sang Chul Kim and Charles Hoopes for graciously providing their UBVI and H images, respectively, of NGC 300. We are most grateful to Karl Gordon for computing new DIRTY models incorporating the LMC2 extinction law, ahead of schedule and upon our request; the corresponding data tables are publicly available on the DIRTY Web site (http://dirty.as.arizona.edu). This research has made use of the NASA/ IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
dc.description.abstractWe investigate the possible origin of the strong radial gradient in the ultraviolet-to-infrared ratio in the nearby late-type spiral galaxy NGC 300 and emphasize the importance of local variations in the geometry of the interstellar medium, concluding that they cannot be neglected with respect to metallicity effects. This analysis is based on a combination of maps obtained both from space using GALEX (1350 to 2750 Å) and Spitzer (3-160 μm) and from the ground (UBVRI, Hα, and Hβ). We select ionizing stellar clusters associated with H II regions of widely varying morphologies and derive their fundamental parameters from population synthesis fitting of their spectral energy distributions, carefully measured to eliminate local background emission accurately. From these fits, we conclude that the stellar extinction law is highly variable in the line of sight of young clusters of similar ages. In the particular model geometry that we consider most appropriate to the sampled regions, we checked that our findings are not significantly altered by the correct treatment of radiative transfer effects. The variations are systematic in nature, in the sense that extinction laws of the Milky Way or LMC type, with a prominent 2175 Å absorption feature and a modest far-ultraviolet slope, are associated with compact H II regions (the compactness being quantified in two different ways), while clusters surrounded by diffuse H II regions follow extinction laws of the 30 Doradus or SMC type, with a weaker 2175 Å feature and a steeper far-ultraviolet rise. The Calzetti starburst attenuation law, although most often degenerate with the 30 Doradus extinction law, overpredicts ionizing photon fluxes by large amounts. We also find that the extinction law variations are correlated with the column density of dust species emitting in the near- and mid-infrared. Finally, we briefly discuss the nebular to stellar extinction ratios and the excitation of aromatic band carriers, invalidating their claimed association with cold dust.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/35934
dc.identifier.doi10.1086/432707
dc.identifier.issn0004-637X
dc.identifier.officialurlhttp://dx.doi.org/10.1086/432707
dc.identifier.relatedurlhttp://iopscience.iop.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/51775
dc.issue.number1
dc.journal.titleAstrophysical journal
dc.language.isoeng
dc.page.final252
dc.page.initial227
dc.publisherAmerican Astronomical Society
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordSmall-magellanic-cloud
dc.subject.keywordStar-forming galaxies
dc.subject.keywordH-II-regions
dc.subject.keywordSculptor group galaxies
dc.subject.keywordDiffuse ionized-gas
dc.subject.keywordInterstellar dust
dc.subject.keywordUltraviolet extinction
dc.subject.keywordStarburst galaxies
dc.subject.keywordSupernova-remnants
dc.subject.keywordHII-regions
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleExtinction law variations and dust excitation in the spiral galaxy NGC 300
dc.typejournal article
dc.volume.number632
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