Role of magnetic fields in the evolution of five dark cloud complexes

Details Role of magnetic fields in the evolution of five dark cloud complexes Role of magnetic fields in the evolution of five dark cloud complexes

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977aj.....82..198v&link_type=abstract

Astronomical Journal, vol. 82, Mar. 1977, p. 198-208.

Astronomy and Astrophysics

Astronomy

60

Hydrogen Clouds, Magnetic Effects, Nebulae, Stellar Evolution, Astronomical Maps, Cloud Physics, Infrared Astronomy, Interstellar Matter, Magnetic Field Configurations, Magnetic Fields, Optical Polarization, Spiral Galaxies, Stellar Gravitation, Stellar Magnetic Fields

Scientific paper

Results are discussed for previously published optical polarization and infrared mapping surveys of five dark cloud complexes (Rho Ophiuchi, R Corona Austrina, Lynds 1450, Lynds 1630, and Lynds 1551). The results are discussed in the context of likely scenarios for the evolution of these clouds, with particular emphasis on the role of magnetic fields in the evolution. An attempt is made to evaluate what factors are important in determining the ability of massive clouds to form stars.

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