Faint companions in the close environment of star-forming dwarf galaxies: possible overlooked starburst triggers?

Details Faint companions in the close environment of star-forming dwarf galaxies: possible overlooked starburst triggers? Faint companions in the close environment of star-forming dwarf galaxies: possible overlooked starburst triggers?

2001-10-03

arxiv.org/abs/astro-ph/0110082v1

"Dwarf Galaxies and their Environment", Eds. K.S. de Boer, R.-J. Dettmar, U. Klein; Bad Honnef, Germany, 23-27 January 2001; S

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures; also available at http://www.astro.uni-bonn.de/~webgk/dgeproc/dge239.ps.gz

Scientific paper

Using the NASA Extragalactic Database, we have searched the close environment of 98 star-forming dwarf galaxies (SFDGs) from field- and low density environments for companion galaxies. Most of the found companions are dwarf galaxies, previously disregarded in environmental studies of SFDGs. Using a subsample at low redshifts, cz < 2000 km/s, i.e. less biased against dwarf companions, we find that 30% of the SFDGs have close companions within a projected linear separation s_p < 100 kpc and a redshift difference of (Delta cz) < 500 km/s. This fraction must be considered a lower limit, given the incompleteness of the available data sets and the non-negligible frequency of HI clouds in the vicinity of SFDGs, so that the majority of SFDGs should not be considered isolated. The redshift differences between companion candidates and sample SFDGs are typically smaller than ~250 km/s and concentrated towards lower values. This is similarly observed for dwarf satellites of spiral galaxies and suggests a physical association between the companion candidates and the sample SFDGs. SFDGs with a close companion do not show significant differences in their H(beta) equivalent widths and B-V colours as compared to isolated ones. However, the available data do not allow to rule out close dwarf companions as an influencing factor for star formation activity.

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