Magnetic fields in massive cloud cores - Comparison of MILLIPOL and IRAS results

Details Magnetic fields in massive cloud cores - Comparison of MILLIPOL and IRAS results Magnetic fields in massive cloud cores - Comparison of MILLIPOL and IRAS results

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...411..708k&link_type=abstract

Astrophysical Journal - Part 1 (ISSN 0004-637X), vol. 411, no. 2, p. 708-719.

Astronomy and Astrophysics

Astronomy

29

H Ii Regions, Infrared Astronomy Satellite, Interstellar Magnetic Fields, Interstellar Matter, Molecular Clouds, Star Formation, Comparison, Cosmic Dust, Morphology, Polarization Characteristics

Scientific paper

The MILLIPOL polarimeter has been used to obtain 30-arcsec resolution 1300-micron data toward 10 cloud cores; the seven that were detected are associated with compact H II regions in massive molecular clouds. Cloud-core axis ratios and position angles were derived by examining the morphologies of IRAS-traced dust opacity structures. The MILLIPOL-detected cloud cores exhibit 1.5-3.2 core axis ratio values. The magnetic field is found to be generally perpendicular to the core dust distributions.

Affiliated with

Also associated with

No associations

Rating

Magnetic fields in massive cloud cores - Comparison of MILLIPOL and IRAS results does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Magnetic fields in massive cloud cores - Comparison of MILLIPOL and IRAS results, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic fields in massive cloud cores - Comparison of MILLIPOL and IRAS results will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1069375