Study of Stellar Populations in Interacting Systems of SBS Galaxies

Details Study of Stellar Populations in Interacting Systems of SBS Galaxies Study of Stellar Populations in Interacting Systems of SBS Galaxies

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mas..conf..397f&link_type=abstract

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

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We are carrying out a project for studying all the Second Byurakan Survey (SBS) interacting systems of galaxies at z < 0.1. The objectives of this project are: (1) to link the histories of the star formation and nuclear activity in these systems with the morphologic type of the interacting galaxies; (2) to settle upper limits to the age of the induced starbursts using the Hα images, which relate with the dynamical time of the interaction; (3) to infer the mass of the stars which are crucial for understanding the physical properties of the perturbed interstellar medium.

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