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Panchromatic radiation from galaxies as a probe of galaxy formation and evolution

Published online by Cambridge University Press:  17 August 2012

Michael Rowan-Robinson
Michael Rowan-Robinson*
Affiliation:
Astrophysics Group, Blackett Laboratory, Imperial College, London SW7 2AZ email: [email protected]
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Abstract

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I review work on modelling the infrared and submillimetre SEDs of galaxies. The underlying physical assumptions are discussed and spherically symmetric, axisymmetric, and 3-dimensional radiative transfer codes are reviewed. Models for galaxies with Spitzer IRS data and for galaxies in the Herschel-Hermes survey are discussed. Searches for high redshift infrared and submillimetre galaxies, the star formation history, the evolution of dust extinction, and constraints from source-counts, are briefly discussed.

Keywords

infrared galaxiesradiative transferstar formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S284: The Spectral Energy Distribution of Galaxies , September 2011 , pp. 446 - 455
Copyright
Copyright © International Astronomical Union 2012

References

Amblard, A., et al. 2011, Nature, 470, 510CrossRefGoogle Scholar
Bell, E. F. 2003, ApJ, 586, 794CrossRefGoogle Scholar
Bethermin, M., et al. 2011, AA, 258, 4CrossRefGoogle Scholar
Blain, A. W. 1996, MNRAS, 283, 1340CrossRefGoogle Scholar
Bruzual, A. G. & Charlot, S. 1993, ApJ, 405, 538CrossRefGoogle Scholar
Chapman, S., et al. 2005, ApJ, 622, 772CrossRefGoogle Scholar
Cox, P., et al. 2011, ApJ, 740, 63CrossRefGoogle Scholar
Dale, D. A., Helou, G., Contursi, A., Silbermann, N. A., & Kolhatkar, S. 2001, ApJ, 549, 215.CrossRefGoogle Scholar
Dopita, M. A., et al. 2005, ApJ, 619, 755CrossRefGoogle Scholar
Dopita, M. A., et al. 2006a, ApJ 647, 244CrossRefGoogle Scholar
Dopita, M. A., et al. 2006b, ApJS 167, 177CrossRefGoogle Scholar
Dullemond, C. P. & van Bemmel, I. M. 2005, A&A, 436, 47Google Scholar
Efstathiou, A. & Siebenmorgen, R. 2009, A&A, 502, 541Google Scholar
Efstathiou, A. & Rowan-Robinson, M. 1995, MNRAS, 273, 649CrossRefGoogle Scholar
Efstathiou, A. & Rowan-Robinson, M. 2003, MNRAS, 343, 322CrossRefGoogle Scholar
Efstathiou, A., Rowan-Robinson, M. & Siebenmorgen, R. 2000, MNRAS, 313, 734CrossRefGoogle Scholar
Franceschini, A., Mazzei, P., de Zotti, G., & Danese, L. 1994, ApJ, 427, 140CrossRefGoogle Scholar
Granato, G.L. & Danese, L. 1994, MNRAS, 268, 235CrossRefGoogle Scholar
Groves, B., et al. 2008, ApJS, 176, 438CrossRefGoogle Scholar
Hoenig, S. F., Beckert, T., Ohnaka, K. & Weigelt, G. 2006, A&A, 452, 459Google Scholar
Hopkins, A. M. 2007, in ‘At the Edge of the Universe’, eds. Afonso, J. et al. , ASP Conf. Ser. 380, 423Google Scholar
Kruegel, E. & Siebenmorgen, R. 1994, A&A, 282, 407Google Scholar
Leung, C. M. 1975, ApJ, 199, 340CrossRefGoogle Scholar
Misiriotis, A., et al. 2001, A&A, 372, 775Google Scholar
Negrello, M., et al. 2010, Science, 330, 800CrossRefGoogle Scholar
Nenkova, M., Ivezic, Z. & Elitzur, M. 2002, ApJ, 570, L9.CrossRefGoogle Scholar
Nenkova, M., Ivezic, Z. & Elitzur, M. 2008, ApJ, 685, 160CrossRefGoogle Scholar
O'Halloran, B., et al. 2010, A&A, 518, L58.Google Scholar
Oliver, S., et al. 2010, A&A, 518, L21.Google Scholar
Pier, G. L. & Krolik, J. 1992, ApJ, 401, 99CrossRefGoogle Scholar
Piovan, L., Tantalo, R., & Chiosi, C. 2006, MNRAS, 366, 923.CrossRefGoogle Scholar
Popescu, C. C., et al. 2000, A&A, 362, 138Google Scholar
Popescu, C. C., et al. 2011, A&A, 527, 109Google Scholar
Rowan-Robinson, M. 1980, ApJS 44, 403CrossRefGoogle Scholar
Rowan-Robinson, M. 1982, in ‘Submillimetre Wave Astronomy’, eds. Beckman, J.E. and Phillips, J.P. (CUP), p.47Google Scholar
Rowan-Robinson, M. & Harris, S. 1982, MNRAS, 200, 197CrossRefGoogle Scholar
Rowan-Robinson, M. & Harris, S. 1983, MNRAS, 202, 767, 797CrossRefGoogle Scholar
Rowan-Robinson, M. & Crawford, J. 1989, MNRAS, 238, 523CrossRefGoogle Scholar
Rowan-Robinson, M., et al. 1991, Nature, 351, 719CrossRefGoogle Scholar
Rowan-Robinson, M. et al. 1993, MNRAS, 261, 513CrossRefGoogle Scholar
Rowan-Robinson, M. 1992, MNRAS 258, 787CrossRefGoogle Scholar
Rowan-Robinson, M. 1995, MNRAS, 272, 737Google Scholar
Rowan-Robinson, M. et al. 1997, MNRAS, 289, 490CrossRefGoogle Scholar
Rowan-Robinson, M. 2001, ApJ, 549, 745CrossRefGoogle Scholar
Rowan-Robinson, M. 2003a, MNRAS, 344, 13CrossRefGoogle Scholar
Rowan-Robinson, M. 2003b, MNRAS, 345, 819CrossRefGoogle Scholar
Rowan-Robinson, M., et al. 2008, MNRAS, 386, 697CrossRefGoogle Scholar
Rowan-Robinson, M. 2009, MNRAS, 394, 117CrossRefGoogle Scholar
Rowan-Robinson, M. & Efstathiou, A. 2009, MNRAS, 399, 615CrossRefGoogle Scholar
Rowan-Robinson, M. & Wang, L. 2010, MNRAS, 406, 720Google Scholar
Rowan-Robinson, M. et al. 2010, MNRAS, 409, 2CrossRefGoogle Scholar
Schartmann, M., et al. 2005, A&A, 437, 861Google Scholar
Schartmann, M., et al. 2008, A&A, 482, 67Google Scholar
Siebenmorgen, R. & Krugel, E. 2007, A&A, 461, 445Google Scholar
Silva, L., Granato, G. L., Bressan, A., & Danese, L. 1998, ApJ, 509, 103CrossRefGoogle Scholar
Spoon, H., et al. 2007, ApJL, 654, L49.CrossRefGoogle Scholar
Takagi, T., Arimoto, N., & Hanami, H. 2003, MNRAS, 340, 813CrossRefGoogle Scholar
Tuffs, R. J., et al. 2004, A&A, 419, 821Google Scholar
Valiante, E., et al. 2009, ApJ, 701, 1814CrossRefGoogle Scholar
Whitney, B. A., et al. 2003, ApJ, 591, 1049CrossRefGoogle Scholar
Whitney, B. A., et al. 2004, ApJ, 617, 1177CrossRefGoogle Scholar
Yorke, H. W. & Kruegel, E. 1977, A&A 54, 183Google Scholar