descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Other literature type 01 Jan 1994 English Publisher:Springer NetherlandsJournal:Symposium - International Astronomical Union, volume 161, pages 589-591 (issn: 0074-1809,

Authors: K.-H. Schmidt; T. Boller;

doi: 10.1007/978-94-011-1146-1_123 , 10.1017/s0074180900048130

Dust in Nearby DWARF Galaxies

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Abstract

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.

Related Organizations

Max Planck Institute for Extraterrestrial Physics
Germany
Max Planck Society
Germany

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