A study of the 2 MON star formation region - Selection of interstellar dust clouds

Details A study of the 2 MON star formation region - Selection of interstellar dust clouds A study of the 2 MON star formation region - Selection of interstellar dust clouds

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...22g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, May-June 1986, p. 22-29. In Russian.

Astronomy and Astrophysics

Astronomy

1

Cosmic Dust, Interstellar Matter, Star Formation, Astronomical Catalogs, Astronomical Maps, Early Stars, Interstellar Extinction, Supernova Remnants

Scientific paper

Interstellar dust clouds of various density have been selected in the direction of the Rosette nebula using a catalog of B, V magnitudes and spectral types of O, B, A stars. The parameters of the clouds (absorption, sizes, masses, spatial densities) show that they are the known types of diffuse and dark clouds. The absorption in dark clouds situated within the supernovae remnants exceeds significantly the absorption in the rest of clouds. That may be the result of cloud compression by a shock wave from a supernova explosion.

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