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A low H I column density filament in NGC 2403 : signature of interaction or accretion
(2014-09-25)
Observed H i accretion around nearby galaxies can only account for a fraction of the gas supply needed to sustain the currently observed star formation rates. It is possible that additional accretion occurs in the form of ...
The Radio Continuum-Star Formation Rate Relation in WSRT SINGS Galaxies
(2014-04-02)
We present a study of the spatially resolved radio continuum–star formation rate (RC–SFR) relation using stateof-the-art star formation tracers in a sample of 17 THINGS galaxies. We use SFR surface density (ΣSFR) maps ...