The gas-to-dust ratio in M 31

Details The gas-to-dust ratio in M 31 The gas-to-dust ratio in M 31

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....41...53v&link_type=abstract

Astronomy and Astrophysics, vol. 41, no. 1, June 1975, p. 53, 54. Research supported by the National Research Council.

Astronomy and Astrophysics

Astrophysics

9

Andromeda Galaxy, Cosmic Dust, Galactic Structure, Interstellar Gas, Mass Ratios, Interstellar Extinction, Mass Distribution, Radial Distribution, Spatial Distribution, Ubv Spectra

Scientific paper

The mean gas-to-dust ratio in M 31 is similar to that observed near the
sun. No evidence is found for a radial gradient in the gas-to-dust ratio
within the disk of the Andromeda Nebula.

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