Cambridge University Press, Proceedings of the International Astronomical Union, A30(14), p. 276-276, 2018
DOI: 10.1017/s1743921319004368
Full text: Unavailable
AbstractWe have combined data of the DustPedia project with observations of gas components of the interstellar medium (ISM) and metallicity abundances for late-type DustPedia galaxies to definitively characterize the ISM scaling relations in the Local Universe. In particular, we have focused on the comparison of the dust-to-gas mass ratio with gas phase metallicities.