The Paα Deficit in IRAS 20100-4156

Details The Paα Deficit in IRAS 20100-4156 The Paα Deficit in IRAS 20100-4156

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mas..conf..101v&link_type=abstract

MULTIWAVELENGTH AGN SURVEYS. Proceedings of the Guillermo Haro Conference 2003. Held 8-12 December 2003 in Cozumel, Mexico. Edit

Astronomy and Astrophysics

Astronomy

Scientific paper

IRAS 20100-4156, being one of the most luminous local Ultraluminous Infrared Galaxies (ULIRGs), is one of the best templates for the analysis of high redshift dust enshrouded galaxies. We present the results of a NIR medium resolution spectroscopic study of this object, carried out with SOFI at ESO 3.5m NTT. Our detection of the Paα line provides ideal constraints on the dust extinction, SFR and presence of an AGN.

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