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Dust-to-gas ratio and metallicity gradients in DustPedia galaxies

Published online by Cambridge University Press:  03 March 2020

Simone Bianchi  and
the DustPedia consortium
Simone Bianchi
Affiliation:
INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125, Firenze, Italy email: [email protected]
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Abstract

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Far-infrared photometric observations from the Herschel Space Observatory offer the opportunity to study the dust-to-gas ratio at a resolved scale in nearby galaxies. The amount, and gradient, of solid-phase metals can thus be compared with metallicity measurements in the gas phase. We describe our preliminary work on the topic with data from the DustPedia project.

Keywords

dustextinctiongalaxies: ISMgalaxies: abundancesgalaxies: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 251 - 252
Copyright
© International Astronomical Union 2020

References

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