Two new methods in determining the structure of dark molecular clouds

Details Two new methods in determining the structure of dark molecular clouds Two new methods in determining the structure of dark molecular clouds

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.187..143c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 187, Jan. 1992, p. 143-146.

Astronomy and Astrophysics

Astrophysics

Dark Matter, Interstellar Extinction, Molecular Clouds, Stellar Evolution, Stellar Spectra, Astronomical Models, Emission Spectra, Raman Spectra, Star Formation, T Tauri Stars

Scientific paper

Two methods for determining the structure of dark molecular clouds are
proposed according to principles and relations of physics and astronomy.
Raman spectra are calculated and some unidentified emission lines are
interpreted for the T Tauri-star LkH-alpha 120 which support the method.

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