Grossi, M., Hunt, L. K., Madden, S., Vlahakis, C., Bomans, D. J., Baes, M., Bendo, G. J., Bianchi, S., Boselli, A., Clemens, M., Corbelli, E., Cortese, Luca ORCID: https://orcid.org/0000-0002-7422-9823, Dariush, Aliakbar, Davies, Jonathan Ivor, De Looze, I., di Serego Alighieri, S., Fadda, D., Fritz, J., Garcia-Appadoo, D. A., Gavazzi, G., Giovanardi, C., Hughes, Thomas Marcus, Jones, A. P., Pierini, D., Pohlen, Michael, Sabatini, S., Smith, Matthew William L. ORCID: https://orcid.org/0000-0002-3532-6970, Verstappen, J., Xilouris, E. M. and Zibetti, S. 2010. The Herschel Virgo Cluster Survey* V. Star-forming dwarf galaxies – dust in metal-poor environments [Letter]. Astronomy & Astrophysics 518 , L52. 10.1051/0004-6361/201014653 |
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Abstract
We present the dust properties of a small sample of Virgo cluster dwarf galaxies drawn from the science demonstration phase data set of the Herschel Virgo Cluster Survey. These galaxies have low metallicities (7.8 < 12 + log(O/H) < 8.3) and star-formation rates ≲10-1 yr-1. We measure the spectral energy distribution (SED) from 100 to 500 μm and derive dust temperatures and dust masses. The SEDs are fitted by a cool component of temperature T ≲ 20 K, implying dust masses around 105 and dust-to-gas ratios within the range 10-3–10-2. The completion of the full survey will yield a larger set of galaxies, which will provide more stringent constraints on the dust content of star-forming dwarf galaxies.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Uncontrolled Keywords: | galaxies: dwarf / galaxies: ISM / dust, extinction / infrared: ISM |
Additional Information: | Letter to the editor. Pdf uploaded in accordance with publisher's policy at http://www.sherpa.ac.uk/romeo/issn/0004-6361/ (accessed 16/04/2014) |
Publisher: | EDP Sciences |
ISSN: | 0004-6361 |
Date of First Compliant Deposit: | 30 March 2016 |
Last Modified: | 07 Aug 2024 22:33 |
URI: | https://orca.cardiff.ac.uk/id/eprint/32724 |
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