The gas/dust ratio in M 33

Details The gas/dust ratio in M 33 The gas/dust ratio in M 33

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..744s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Oct. 1985, p. 744-748) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, Sept.-Oc

Astronomy and Astrophysics

Astronomy

Cosmic Dust, Interstellar Gas, Interstellar Matter, Local Group (Astronomy), Neutral Gases, Spiral Galaxies, Astronomical Photometry, Color, Globular Clusters, Hydrogen Clouds, Supergiant Stars

Scientific paper

Using photometric data on blue supergiants and young globular clusters and data on the neutral hydrogen distribution it is found that the mean gas-to-dust ratio in M33 turns out to be NHI/EB-V ≈ 1.5×1021 atom/cm2mag. According to the low gas-to-dust ratio M33 differs considerably from other studied galaxies of the Local Group.

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