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Galaxy Evolution Explorer Ultraviolet Spectroscopy and Deep Imaging of Luminous Infrared Galaxies in the European Large‐Area ISO Survey S1 Field

  • Authors: Denis Burgarella, Véronique Buat, Todd Small, Tom A. Barlow, Samuel Boissier, Armando Gil de Paz, Timothy M. Heckman, Barry F. Madore, D. Christopher Martin, R. Michael Rich, Luciana Bianchi, Yong-Ik Byun, Jose Donas, Karl Forster, Peter G. Friedman, Patrick N. Jelinsky, Young-Wook Lee, Roger F. Malina, Bruno Milliard, Patrick Morrissey, Susan G. Neff, David Schiminovich, Oswald H. W. Siegmund, Alex S. Szalay, Barry Y. Welsh, and Ted K. Wyder

Burgarella et al. 2005 The Astrophysical Journal Letters 619 L63.

  • Provider: AAS Journals

Caption: Fig. 3.

Log of the ﹩L_{\mathrm{IR}\,}/ L_{\mathrm{FUV}\,}﹩ ratio plotted against the UV slope β. Our sample is represented with the same symbols as in Fig. 2, and Goldader et al. (2002) objects are added as crosses. One of them falls within our sample, and the other ones are redder and more extinguished. Most of the objects do not follow the law deduced from the UV observation of starbursts (e.g., Kong et al. 2004 overplotted here): the sample extends upward.

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