Radial dust properties of SINGS galaxies

DOI

We present a detailed analysis of the radial distribution of dust properties in the SINGS sample, performed on a set of ultraviolet (UV), infrared (IR), and HI surface brightness profiles, combined with published molecular gas profiles and metallicity gradients. By applying physical dust models to our radial spectral energy distributions, we have derived radial profiles of the total dust mass surface density, the fraction of the total dust mass contributed by polycyclic aromatic hydrocarbons (PAHs), and the intensity of the radiation field heating the grains.

Cone search capability for table J/ApJ/701/1965/table1 (Sample)

Identifier
DOI http://doi.org/10.26093/cds/vizier.17011965
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/ApJ/701/1965
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/701/1965
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/701/1965
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/ApJ/701/1965
Provenance
Creator Munoz-Mateos J.C.; Gil de Paz A.; Boissier S.; Zamorano J.; Dale D.A.,Perez-Gonzalez P.G.; Gallego J.; Madore B.F.; Bendo G.; Thornley M.D.,Draine B.T.; Boselli A.; Buat V.; Calzetti D.; Moustakas J.; Kennicutt R.C.
Publisher CDS
Publication Year 2011
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Galactic and extragalactic Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics