Infrared polarimetry in the Rho Ophiuchus dark cloud

Details Infrared polarimetry in the Rho Ophiuchus dark cloud Infrared polarimetry in the Rho Ophiuchus dark cloud

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..199w&link_type=abstract

Astronomical Journal, vol. 84, Feb. 1979, p. 199-203. NSF-supported research.

Astronomy and Astrophysics

Astronomy

31

Infrared Astronomy, Line Spectra, Nebulae, Polarimetry, Star Clusters, Carbon Monoxide, Cosmic Dust, Density Distribution, Interstellar Extinction, Molecular Spectra, Self Absorption, Signal To Noise Ratios, Stellar Evolution

Scientific paper

Infrared polarimetry has been obtained of 16 objects in the proposed
region of star formation in the Rho Oph dark cloud. This study is used
along with visual polarimetry, infrared photometry, and molecular line
studies to deduce the cloud morphology around the very young stellar
cluster.

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