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The dust/gas/metallicity scaling relations in the Local Universe

Published online by Cambridge University Press:  03 March 2020

V. Casasola
Affiliation:
INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy email: casasola@arcetri.astro.it
S. Bianchi
Affiliation:
INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy email: casasola@arcetri.astro.it
P. De Vis
Affiliation:
IAS, CNRS, Univ. Paris-Sud, Univ. Paris-Saclay, 91405, Orsay Cedex, France
L. Magrini
Affiliation:
INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy email: casasola@arcetri.astro.it
E. Corbelli
Affiliation:
INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy email: casasola@arcetri.astro.it
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Abstract

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We 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.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

Casasola, V., Cassarà, L. P., Bianchi, S., et al. 2017, A&A, 605, A18 Google Scholar
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Davies, J. I., Baes, M., Bianchi, S., et al. 2017, PASP, 129, 044102 Google Scholar
De Vis, P., Jones, A., Viaene, S., et al. 2019, A&A, 623, A5 Google Scholar
Wang, J., Fu, J., Aumer, M., et al. 2014, MNRAS, 441, 2159 CrossRefGoogle Scholar