The fine structure of the galactic dust cloud distribution near the sun

Details The fine structure of the galactic dust cloud distribution near the sun The fine structure of the galactic dust cloud distribution near the sun

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....44..209t&link_type=abstract

Astronomy and Astrophysics, vol. 44, no. 1, Nov. 1975, p. 209-213.

Astronomy and Astrophysics

Astronomy

7

Cosmic Dust, Density Wave Model, Far Infrared Radiation, Fine Structure, Galactic Structure, Infrared Astronomy, Cloud Physics, Interstellar Extinction, Shock Fronts, Supersonic Flow

Scientific paper

Two very dark clouds in Ophiuchus and Taurus are almost exactly
symmetrical around the sun. A study of the color excess of nearby stars
confirms the idea of a thin elongated cloud linking the two symmetrical
regions. The orientation of this long cloud suggests an aligning
mechanism related to spiral density waves.

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