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Cited by 138Galaxies: Formation, Evolution, PhenomenaAstrophysics and Star Formation StudiesStellar, planetary, and galactic studies

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

DUST HEATING SOURCES IN GALAXIES: THE CASE OF M33 (HERM33ES)

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Boquien, M., Calzetti, D., Combes, F., Henkel, C., Israel, F., Kramer, C., Relaño, M., Verley, S., van der Werf, P., Xilouris, E. M., The HERM33ES Team·2011·The Astronomical Journal
DOI 10.1088/0004-6256/142/4/111
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Abstract

Dust emission is one of the main windows to the physics of galaxies and to star formation as the radiation from young, hot stars is absorbed by the dust and reemitted at longer wavelengths. The recently launched Herschel satellite now provides a view of dust emission in the far-infrared at an unequaled resolution and quality up to 500 μm. In the context of the Herschel HERM33ES open time key project, we are studying the moderately inclined Scd local group galaxy M33 which is located only 840 kpc away. In this article, using Spitzer and Herschel data ranging from 3.6 μm to 500 μm, along with H i , Hα maps, and Galaxy Evolution Explorer ultraviolet data, we have studied the emission of the dust at the high spatial resolution of 150 pc. Combining Spitzer and Herschel bands, we have provided new, inclination-corrected, resolved estimators of the total infrared brightness and of the star formation rate from any combination of these bands. The study of the colors of the warm and cold dust populations shows that the temperature of the former is, at high brightness, dictated by young massive stars but, at lower brightness, heating is taken over by the evolved populations. Conversely, the temperature of the cold dust is tightly driven by the evolved stellar populations.

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  • In nearby spirals, a significant fraction of the 24um flux, particularly in bulges and inner disks, arises from dust heated by older stars rather than embedded HII regions.

    “In nearby spirals, analyses of the radial energy budget find that a significant fraction of the 24 µ m flux, particularly in bulges and inner disks, arises from dust heated by older stars rather than embedded HII regions (e.g., Boquien et al. 2011; Leroy et al. 2012).”

    From The Panchromatic Hubble Andromeda Southern Treasury (PHAST). II. The Spatially Resolved Recent Star Formation History in M31 (2026) · cites this paper as Boquien et al. 2011

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Metadata

Authors
Boquien, M., Calzetti, D., Combes, F., Henkel, C., Israel, F., Kramer, C., Relaño, M., Verley, S., van der Werf, P., Xilouris, E. M., & The HERM33ES Team
Affiliations
  • Centre National de la Recherche Scientifique (FR)
  • University of Massachusetts Amherst (US)
  • Observatoire de Paris (FR)
  • Max Planck Institute for Radio Astronomy (DE)
  • Leiden University (NL)
  • Instituto de Radioastronomía Milimétrica (ES)
  • Universidad de Granada (ES)
  • National Observatory of Athens (GR)
Corresponding author
  • Boquien, M.
  • Henkel, C.
  • Kramer, C.
  • van der Werf, P.
ORCID
Venue
The Astronomical Journal
Publisher
American Astronomical Society
Published
2011-09-01
Volume
142
Issue
4
Pages
111
ISSN
  • 0004-6256 (ISSN-L)
  • 1538-3881
DOI
10.1088/0004-6256/142/4/111
OpenAlex
W2068388304
Cited by
138
References
1
Citations by year
2026: 1 · 2024: 4 · 2022: 5 · 2021: 5 · 2020: 7 · 2019: 4 · 2018: 7 · 2017: 9 · 2016: 16 · 2015: 13 · 2014: 32 · 2013: 14 · 2012: 16
FWCI
11.39
Type
journal article
Language
en
Open access
Locations
  • The Astronomical Journal (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • HAL (submittedVersion)
  • ScholarWorks@UMassAmherst (University of Massachusetts Amherst) (submittedVersion)
  • arXiv (Cornell University)
  • The Astrophysical Journal
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords
M33, dust heating, far-infrared dust emission, star formation rate, dust temperature, stellar populations, young massive stars, evolved stellar populations, Spitzer, Local Group galaxies

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