Environment status of blue compact galaxies and trigger of star formation

Details Environment status of blue compact galaxies and trigger of star formation Environment status of blue compact galaxies and trigger of star formation

2001-04-20

arxiv.org/abs/astro-ph/0104334v1

Astronomy and Astrophysics

Astrophysics

22 pages, 7 figures, accepted to A&A on March 26, 2001

Scientific paper

10.1051/0004-6361:20010555

(abridged) The work studies active star formation (SF) and a possible trigger of SF bursts due to gravitational interaction. Following the study by Taylor et al. we extend the search for possible disturbing galaxies of various masses to a much larger sample of 86 BCGs from the sky region of Second Byurakan survey. The sample under study is separated by the criteria: EW([O III]5007 > 45 A and V < 6,000 km/s and should be representative of all low-mass galaxies which experience SF bursts. We argue that the moderate tidal disturbers should be taken into account, and incorporate the respective range of distances in the search for disturbing neighbours. The majority of the neighbours in the vicinity of the studied BCGs are found through the study of their environment among UZC galaxies, and the follow-up careful search of the fainter galaxies in the NED database. For the remaining BCGs, the neighbouring galaxies are found based on the results of the 6-m telescope spectroscopy. By studing the data on the radial velocities of galaxies in the vicinity of BCGs we found: 1) 33 of the studied BCGs (38.5 %) are associated with significantly brighter galaxies (DB > 1.5 mag); 2) 23 BCGs (26.5%) have neighbours either of comparable or significantly lower brightness; 3) 14 of the studied BCGs (16%) with no evident associated galaxy are either certain, or probable, mergers. We conclude that in \~80% (or more) BCGs from the studied sample, the SF bursts are triggered either by tidal action of various strengths from other galaxies, or due to mergers of low-mass galaxies. We briefly discuss the implications of our main conclusion for evolutionary links of BCGs to other types of low-mass galaxies. Among the ``isolated'' BCGs (without a bright neighbour) 43+-10% are probably disturbed by dwarf galaxies and 26+-8% have a merger morphology.

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