Sign in

Variations in the Σ_{\rm SFR} {-} Σ_{\rm mol} {-} Σ_{\rm \star} plane across galactic environments in PHANGS galaxies

By I. Pessa and others
There exists some consensus that stellar mass surface density (\Sigma_{*}) and molecular gas mass surface density (\Sigma_{\rm mol}) are the main quantities responsible for locally setting the star formation rate. This regulation is inferred from locally resolved scaling relations between these two quantities and the star formation rate surface density... Show more
March 29, 2022
=
0
Loading PDF…
Loading full text...
Similar articles
Loading recommendations...
=
0
x1
Variations in the $Σ_{\rm SFR} {-} Σ_{\rm mol} {-} Σ_{\rm \star}$ plane across galactic environments in PHANGS galaxies
Click on play to start listening