Magnetic Field Continuity from 100 to 0.1 Parsec Scales

Details Magnetic Field Continuity from 100 to 0.1 Parsec Scales Magnetic Field Continuity from 100 to 0.1 Parsec Scales

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21334706l&link_type=abstract

American Astronomical Society, AAS Meeting #213, #347.06; Bulletin of the American Astronomical Society, Vol. 41, p.483

Astronomy and Astrophysics

Astronomy

Scientific paper

The biggest open questions in star formation concern mechanisms that oppose gravitational collapse and regulate star formation. While turbulence and magnetic fields are almost ubiquitous in molecular clouds, their relative importance is often the key contrasting assumption between the major star formation theories. Using multi-wavelength and multi-scale polarimetry observations from JCMT, CSO, SMA, and optical telescopes we present observational evidence of magnetic fields being a crucial player over a large range of scales.

Affiliated with

Also associated with

No associations

Rating

Magnetic Field Continuity from 100 to 0.1 Parsec Scales 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 Field Continuity from 100 to 0.1 Parsec Scales, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic Field Continuity from 100 to 0.1 Parsec Scales will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1699870