Byurakan-IRAS Galaxy Pairs as Indicators of Starburst and Galaxy Evolution

Details Byurakan-IRAS Galaxy Pairs as Indicators of Starburst and Galaxy Evolution Byurakan-IRAS Galaxy Pairs as Indicators of Starburst and Galaxy Evolution

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..124m&link_type=abstract

Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267

Astronomy and Astrophysics

Astronomy

Infrared: Galaxies, Galaxies: Interactions, Galaxies: Starburst, Galaxies: Active, Galax9 Ies: Evolution

Scientific paper

The Byurakan-IRAS galaxies (BIG objects; Mickaelian 1995) are the result of a project of optical identifications of IRAS Point Source Catalog (PSC; IRAS 1988) in a 1500 square degree high-galactic latitude (|b|>15°) area based on the Digitized Sky Survey (DSS) images and the Digitized First Byurakan Survey (DFBS, or digitized Markarian survey) low-dispersion spectra. As a result, 1278 galaxies have been identified (as well as galactic objects, Byurakan-IRAS Stars [BIS]), including 42 PSC sources identified with 103 galaxies that make up 30 physical pairs and 12 multiples.

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