SED fitting of nearby galaxies in the Herschel Reference Survey

Ciesla, L., Boselli, A., Buat, V., Cortese, L., Auld, Robbie, Baes, M., Bendo, G. J., Bianchi, S., Bock, J., Bomans, D. J., Bradford, M., Castro-Rodriguez, N., Chanial, P., Charlot, S., Clemens, M., Clements, D., Corbell, E., Cooray, A., Cormie, D., Dariush, A., Davies, J., de Looze, I., di Serego Alighieri, S., Dwek, E., Eales, Stephen Anthony ORCID: https://orcid.org/0000-0002-7394-426X, Elbaz, D., Fadda, D., Fritz, J., Galametz, M., Galliano, F., Garcia-Appadoo, D. A., Gavazzi, G., Gear, Walter Kieran ORCID: https://orcid.org/0000-0001-6789-6196, Giovanardi, C., Glenn, J., Gomez, Haley ORCID: https://orcid.org/0000-0003-3398-0052, Griffin, Matthew Joseph ORCID: https://orcid.org/0000-0002-0033-177X, Grossi, M., Hony, S., Hughes, T. M., Hunt, L., Isaak, K., Jones, A., Levenson, L., Lu, N., Madden, S. C., O'Halloran, B., Okumura, K., Oliver, S., Page, M., Panuzzo, P., Papageorgiou, Andreas, Parkin, T., Perez-Fournon, I., Pierini, D., Pohlen, M., Rangwala, N., Rigby, E., Roussel, H., Rykala, A., Sabatini, S., Sacchi, N., Sauvage, M., Schulz, B., Schirm, M., Smith, Matthew ORCID: https://orcid.org/0000-0002-3532-6970, Spinoglio, L., Stevens, J., Sundar, S., Symeonidis, M., Trichas, M., Vaccari, M., Verstappen, J., Vigroux, L., Vlahakis, C., Wilson, C., Wozniak, H., Wright, G., Xilouris, E. M., Zeilinger, W., Zibetti, S., Heydari-Malayeri, M., Samadi, R. and Valls-Gabaud, D. 2010. SED fitting of nearby galaxies in the Herschel Reference Survey. Presented at: SF2A-2010: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, Marseille, France,

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Abstract

We compute UV to radio continuum spectral energy distributions of 51 nearby galaxies recently observed with SPIRE onboard Herschel and present infrared colours (in the 25-500 μm spectral range). SPIRE data of normal galaxies are well reproduced with a modified black body (β=2) of temperature T≃q 20 K. In ellipticals hosting a radio galaxy, the far-infrared (FIR) emission is dominated by the synchrotron nuclear emission. The colour temperature of the cold dust is higher in quiescent E-S0a than in star-forming systems probably because of the different nature of their dust heating sources (evolved stellar populations, X-ray, fast electrons) and dust grain properties.

Item Type:	Conference or Workshop Item (Paper)
Schools:	Physics and Astronomy
Last Modified:	03 Dec 2022 11:58
URI:	https://orca.cardiff.ac.uk/id/eprint/14933

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