The Environmental Dependence of Star Formation in the Nearby Universe

Abstract

We have investigated how the incidence of star-forming galaxies varies with the environment using a volume-limited sample of nearby galaxy spectra extracted from the 2dF Galaxy Redshift Survey. The environment is characterized by the local number density of galaxies, corrected for sample incompleteness and border effects. Using the equivalent widths of [O II]$λ$3727 and H$δ$ we discriminate the star-forming galaxies in two classes, starbursts and ordinary star-forming galaxies, and evaluate their properties as a function of the local density. We show that the fraction of ordinary star-forming galaxies decreases regularly with increasing density, indicating that star formation is sensitive to the environment for all range of densities present in the sample. The fraction of starbursts is approximately independent of the density and, consequently, the fraction of starbursts relative to star-forming galaxies increases with local density. This suggests that a mechanism that acts everywhere, like tidal interactions, is the responsible for triggering starbursts. We also show that while the mean EW(H$α$) of ordinary star-forming galaxies is progressively reduced as density increases, for starbursts it suffers a strong decrease at densities corresponding to scales of $ρ^{-1/3} \sim 2.5 ~h^{-1}$ Mpc. A visual inspection of starburst images in the {\it Digital Sky Survey} reveals that this corresponds to a change in the morphology of starburst galaxies, from mainly apparently normal spirals and galaxies with apparently compact morphologies at low densities, to tidally distorted spirals at high densities.