Optical polarization measurements in the vicinity of nearby star-forming complexes. I - The LYNDS 1641 molecular cloud

Details Optical polarization measurements in the vicinity of nearby star-forming complexes. I - The LYNDS 1641 molecular cloud Optical polarization measurements in the vicinity of nearby star-forming complexes. I - The LYNDS 1641 molecular cloud

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aj.....96..680v&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 96, Aug. 1988, p. 680-694, 805. NSF-NASA-supported research.

Astronomy and Astrophysics

Astronomy

57

Molecular Clouds, Optical Polarization, Polarimetry, Star Formation, Gravitational Collapse, Interstellar Magnetic Fields, Polarization Characteristics, Protostars, Tables (Data)

Scientific paper

Optical polarization results for 219 stars located in the vicinity of the Lynds 1641 giant molecular cloud are presented. The data indicate that L 1641 is representative of a class of star-forming complexes in which the magnetic field has played an incidental role during the global cloud-collapse phases. It is suggested that the magnetic field may control the direction of collimated mass outflows associated with young stellar objects.

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