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Dust in Nearby Dwarf Galaxies
Published online by Cambridge University Press: 26 July 2016
Extract
The aim of the present paper is to look for the gas-to-dust ratio in different types of galaxies and for a correlation between this ratio and the metallicity in dwarf galaxies. The recent compilation of data on nearby galaxies by Schmidt & Boller (1992, hereinafter SB) including HI and dust masses from IRAS data is used to estimate the gas-to-dust ratio in galaxies of a volume-limited sample.
- Type
- Part Twelve: Properties of Nearby Galaxies
- Information
- Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 589 - 591
- Copyright
- Copyright © Kluwer 1994