One feature of interstellar reddening lines

Details One feature of interstellar reddening lines One feature of interstellar reddening lines

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...25s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, May-June 1988, p. 25-28. In Russian.

Computer Science

Interstellar Radiation, Red Shift, Stellar Composition, Cosmochemistry, Interstellar Chemistry, Line Spectra, Solar Neighborhood, Ubv Spectra

Scientific paper

It is demonstrated that interstellar reddening lines have a complex structure. The possibility that this structure is related to differences in stellar chemical composition is discussed. It is shown that the set of points on the two-index (U-V), (B1-V) diagram constituting the reddening line breaks down into several subsets in the direction perpendicular to the reddening line. It is concluded that the most probable cause of the separation of the interstellar reddening line is differences in the chemical composition of Galactic-disk stars close to the sun.

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