The Lick galaxy counts, the local interstellar absorption and molecular hydrogen

Details The Lick galaxy counts, the local interstellar absorption and molecular hydrogen The Lick galaxy counts, the local interstellar absorption and molecular hydrogen

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...105..159s&link_type=abstract

Astronomy and Astrophysics, vol. 105, no.1, Jan. 1982, p. 159-163.

Astronomy and Astrophysics

Astrophysics

25

Galaxies, Hydrogen, Interstellar Extinction, Molecular Clouds, Atmospheric Density, Cosmic Dust, Gas Density, Interstellar Gas, Radiation Absorption

Scientific paper

An interpretation of the relationships between the Lick galaxy counts and atmospheric and galactic extinction leads to a simple picture in which apparent variations in the gas-to-dust ratio are mainly due to molecular hydrogen. Parameters entering into these relationships are re-evaluated. Finally, this makes it possible to map the large-scale distribution of molecular hydrogen in the local interstellar medium.

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