UBV photometry of the NGC 2805-NGC 2814-NGC 2820-Mk 108 group of galaxies

Details UBV photometry of the NGC 2805-NGC 2814-NGC 2820-Mk 108 group of galaxies UBV photometry of the NGC 2805-NGC 2814-NGC 2820-Mk 108 group of galaxies

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994arep...38..597a&link_type=abstract

Astronomy Reports, Volume 38, Issue 5, September 1994, pp.597-604

Astronomy and Astrophysics

Astronomy

1

Scientific paper

UBV photometry of Ho 124 group galaxies NGC 2805, NGC 2814, NGC 2820, and Mk 108 was carried out. Blue condensations ("stellar aggregates") were singled out in central regions and spirals of these galaxies. A two-color diagram location of these condensations corresponds to a region occupied by young objects 10^6^ - 10^7^ years old according to models of galactic photometric evolution. The enhanced star formation rate in galaxies of the Ho 124 group is most likely due to intergalactic interaction that causes distortions in their symmetry.

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