Distribution of interstellar dust matter in the direction L = 207 deg, B = -3 deg

Details Distribution of interstellar dust matter in the direction L = 207 deg, B = -3 deg Distribution of interstellar dust matter in the direction L = 207 deg, B = -3 deg

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2....3g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Mar.-Apr. 1986, p. 3-12. In Russian.

Physics

1

Cosmic Dust, Interstellar Extinction, Interstellar Matter, Milky Way Galaxy, Molecular Clouds, Stellar Evolution, Galactic Structure

Scientific paper

Interstellar absorption distribution is investigated in the direction of the star formation region 2 Mon (l = 207 + or 2.5 deg; b = - 3 + or - 2.5 deg). Mean curves of interestellar absorption are obtained for seven areas in the investigated region using two methods with different averaging schemes. It is shown that the direction studied is characterized by low mean absorption (1.2-1.4 m/kpc) within the local spiral arm and by the presence of dense interstellar clouds in regions near the galactic plane.

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