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Far-infrared colours of nearby late-type galaxies in the Herschel Reference Survey

A Boselli, L Ciesla, L Cortese, V Buat, M Boquien, GJ Bendo, S Boissier, S Eales, G Gavazzi and TM Hughes, et al. (2012) ASTRONOMY & ASTROPHYSICS. 540.
abstract
We study the far infrared (60-500 mu m) colours of late-type galaxies in the Herschel Reference Survey, a K-band selected, volume limited sample of nearby galaxies. The far infrared colours are correlated with each other, with tighter correlations for the indices that are closer in wavelength. We also compare the different colour indices to various tracers of the physical properties of the target galaxies, such as the surface brightness of the ionising and non-ionising stellar radiation, the dust attenuation and the metallicity. The emission properties of the cold dust dominating the far infrared spectral domain are regulated by the properties of the interstellar radiation field. Consistent with that observed in nearby, resolved galaxies, our analysis shows that the ionising and the non-ionising stellar radiation, including that emitted by the most evolved, cold stars, both contribute to the heating of the cold dust component. This work also shows that metallicity is another key parameter characterising the cold dust emission of normal, late-type galaxies. A single modified black body with a grain emissivity index beta = 1.5 better fits the observed SPIRE flux density ratios S 250/S 350 vs. S 350/S 500 than beta = 2, although values of beta similar or equal to 2 are possible in metal rich, high surface brightness galaxies. Values of beta less than or similar to 1.5 better represent metal poor, low surface brightness objects. This observational evidence provides strong constraints for dust emission models of normal, late type galaxies.
Please use this url to cite or link to this publication:
author
organization
year
type
journalArticle (original)
publication status
published
subject
keyword
galaxies: ISM, STAR-FORMING GALAXIES, galaxies: spiral, infrared: galaxies, BAND SURFACE PHOTOMETRY, HIGH-REDSHIFT UNIVERSE, GAS MASS-RATIO, INTERSTELLAR DUST, SPIRAL GALAXIES, VIRGO CLUSTER, IRAS GALAXIES, PHYSICAL-PROPERTIES, ASTROPHYSICAL DUST
journal title
ASTRONOMY & ASTROPHYSICS
Astron. Astrophys.
volume
540
article_number
A54
pages
22 pages
Web of Science type
Article
Web of Science id
000303315400068
JCR category
ASTRONOMY & ASTROPHYSICS
JCR impact factor
5.084 (2012)
JCR rank
11/56 (2012)
JCR quartile
1 (2012)
ISSN
0004-6361
DOI
10.1051/0004-6361/201118602
language
English
UGent publication?
yes
classification
A1
copyright statement
I have transferred the copyright for this publication to the publisher
id
2113380
handle
http://hdl.handle.net/1854/LU-2113380
date created
2012-05-25 14:44:09
date last changed
2012-05-30 15:38:37
@article{2113380,
  abstract     = {We study the far infrared (60-500 mu m) colours of late-type galaxies in the Herschel Reference Survey, a K-band selected, volume limited sample of nearby galaxies. The far infrared colours are correlated with each other, with tighter correlations for the indices that are closer in wavelength. We also compare the different colour indices to various tracers of the physical properties of the target galaxies, such as the surface brightness of the ionising and non-ionising stellar radiation, the dust attenuation and the metallicity. The emission properties of the cold dust dominating the far infrared spectral domain are regulated by the properties of the interstellar radiation field. Consistent with that observed in nearby, resolved galaxies, our analysis shows that the ionising and the non-ionising stellar radiation, including that emitted by the most evolved, cold stars, both contribute to the heating of the cold dust component. This work also shows that metallicity is another key parameter characterising the cold dust emission of normal, late-type galaxies. A single modified black body with a grain emissivity index beta = 1.5 better fits the observed SPIRE flux density ratios S 250/S 350 vs. S 350/S 500 than beta = 2, although values of beta similar or equal to 2 are possible in metal rich, high surface brightness galaxies. Values of beta less than or similar to 1.5 better represent metal poor, low surface brightness objects. This observational evidence provides strong constraints for dust emission models of normal, late type galaxies.},
  articleno    = {A54},
  author       = {Boselli, A and Ciesla, L and Cortese, L and Buat, V and Boquien, M and Bendo, GJ and Boissier, S and Eales, S and Gavazzi, G and Hughes, TM and Pohlen, M and Smith, MWL and Baes, Maarten and Bianchi, S and Clements, DL and Cooray, A and Davies, J and Gear, W and Madden, S and Magrini, L and Panuzzo, P and Remy, A and Spinoglio, L and Zibetti, S},
  issn         = {0004-6361},
  journal      = {ASTRONOMY \& ASTROPHYSICS},
  keyword      = {galaxies: ISM,STAR-FORMING GALAXIES,galaxies: spiral,infrared: galaxies,BAND SURFACE PHOTOMETRY,HIGH-REDSHIFT UNIVERSE,GAS MASS-RATIO,INTERSTELLAR DUST,SPIRAL GALAXIES,VIRGO CLUSTER,IRAS GALAXIES,PHYSICAL-PROPERTIES,ASTROPHYSICAL DUST},
  language     = {eng},
  pages        = {22},
  title        = {Far-infrared colours of nearby late-type galaxies in the Herschel Reference Survey},
  url          = {http://dx.doi.org/10.1051/0004-6361/201118602},
  volume       = {540},
  year         = {2012},
}

Chicago
Boselli, A, L Ciesla, L Cortese, V Buat, M Boquien, GJ Bendo, S Boissier, et al. 2012. “Far-infrared Colours of Nearby Late-type Galaxies in the Herschel Reference Survey.” Astronomy & Astrophysics 540.
APA
Boselli, A., Ciesla, L., Cortese, L., Buat, V., Boquien, M., Bendo, G., Boissier, S., et al. (2012). Far-infrared colours of nearby late-type galaxies in the Herschel Reference Survey. ASTRONOMY & ASTROPHYSICS, 540.
Vancouver
1.
Boselli A, Ciesla L, Cortese L, Buat V, Boquien M, Bendo G, et al. Far-infrared colours of nearby late-type galaxies in the Herschel Reference Survey. ASTRONOMY & ASTROPHYSICS. 2012;540.
MLA
Boselli, A, L Ciesla, L Cortese, et al. “Far-infrared Colours of Nearby Late-type Galaxies in the Herschel Reference Survey.” ASTRONOMY & ASTROPHYSICS 540 (2012): n. pag. Print.