Optical Spectra of Dusty Starbursts
Abstract
Description
This contribution presents the optical spectral properties of FIR-luminous galaxies, whose distinctive feature is often the simultaneous presence in the spectra of a strong $\rm Hδ$ line in absorption and of emission lines (e(a) spectra). A discrepancy between the star formation rate estimated from the FIR luminosity and that derived from the $\rm Hα$ luminosity persists even after having corrected the $\rm Hα$ flux for dust according to the observed Balmer decrement. It is shown that the e(a) spectrum can be reproduced assuming a current starburst and dust extinction affecting the youngest stellar populations much more than the older stars.
6 pages, 5 postscript figures, Springer Latex macro. Invited talk, to appear in the proceedings of the meeting "Starbursts Near and Far", Ringberg Castle (D), 10-15 Sep 2000
6 pages, 5 postscript figures, Springer Latex macro. Invited talk, to appear in the proceedings of the meeting "Starbursts Near and Far", Ringberg Castle (D), 10-15 Sep 2000