JINGLE - V. Dust properties of nearby galaxies derived from hierarchical Bayesian SED fitting

Autor: Gioacchino Accurso, Jong Chul Lee, Ting Xiao, Lihwai Lin, Isabella Lamperti, Ho Seong Hwang, Michał J. Michałowski, Matthew Smith, Amélie Saintonge, Elias Brinks, Toby Brown, Ilse De Looze, Christine D. Wilson, Thomas G. Williams, David L. Clements, Christopher J. R. Clark, David Henry william Glass, C. Yang, Martin Bureau, Mark Sargent, Stephen Anthony Eales
Jazyk: angličtina
Rok vydání: 2019
Předmět:
Stellar mass
INFRARED-EMISSION
Extinction (astronomy)
FOS: Physical sciences
F500
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Astronomy & Astrophysics
01 natural sciences
0103 physical sciences
0201 Astronomical and Space Sciences
Emissivity
Astrophysics::Solar and Stellar Astrophysics
Black-body radiation
ISM [submillimetre]
COLD DUST
MAIN-SEQUENCE
010303 astronomy & astrophysics
evolution [galaxies]
Astrophysics::Galaxy Astrophysics
QB
Cosmic dust
Physics
Science & Technology
ISM [galaxies]
extinction
010308 nuclear & particles physics
Star formation
JCMT LEGACY SURVEY
Astronomy and Astrophysics
HERSCHEL-ATLAS
Astrophysics - Astrophysics of Galaxies
Galaxy
submillimetre: ISM
MODEL
SPECTRAL ENERGY-DISTRIBUTION
Physics and Astronomy
TEMPERATURE-DEPENDENCE
Space and Planetary Science
GAS
Astrophysics of Galaxies (astro-ph.GA)
Physical Sciences
Spectral energy distribution
dust
Astrophysics::Earth and Planetary Astrophysics
dust
extinction

galaxies: evolution
galaxies: ISM
INTERSTELLAR DUST
Zdroj: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN: 0035-8711
1365-2966
Popis: We study the dust properties of 192 nearby galaxies from the JINGLE survey using photometric data in the 22-850micron range. We derive the total dust mass, temperature T and emissivity index beta of the galaxies through the fitting of their spectral energy distribution (SED) using a single modified black-body model (SMBB). We apply a hierarchical Bayesian approach that reduces the known degeneracy between T and beta. Applying the hierarchical approach, the strength of the T-beta anti-correlation is reduced from a Pearson correlation coefficient R=-0.79 to R=-0.52. For the JINGLE galaxies we measure dust temperatures in the range 17-30 K and dust emissivity indices beta in the range 0.6-2.2. We compare the SMBB model with the broken emissivity modified black-body (BMBB) and the two modified black-bodies (TMBB) models. The results derived with the SMBB and TMBB are in good agreement, thus applying the SMBB, which comes with fewer free parameters, does not penalize the measurement of the cold dust properties in the JINGLE sample. We investigate the relation between T and beta and other global galaxy properties in the JINGLE and Herschel Reference Survey (HRS) sample. We find that beta correlates with the stellar mass surface density (R=0.62) and anti-correlates with the HI mass fraction (M(HI)/M*, R=-0.65), whereas the dust temperature correlates strongly with the SFR normalized by the dust mass (R=0.73). These relations can be used to estimate T and beta in galaxies with insufficient photometric data available to measure them directly through SED fitting.
MNRAS in press, 31 pages
Databáze: OpenAIRE