pith. machine review for the scientific record. sign in

arxiv: 1304.6739 · v1 · submitted 2013-04-24 · 🌌 astro-ph.SR

Recognition: unknown

The Magnetic Field Morphology of the Class 0 Protostar L1157-mm

Authors on Pith no claims yet
classification 🌌 astro-ph.SR
keywords fieldmagneticcarmaobservationsprotostararoundclassdifferent
0
0 comments X
read the original abstract

We present the first detection of polarization around the Class 0 low-mass protostar L1157-mm at two different wavelengths. We show polarimetric maps at large scales (10" resolution at 350 um) from the SHARC-II Polarimeter and at smaller scales (1.2"-4.5" at 1.3 mm) from the Combined Array for Research in Millimeter-wave Astronomy (CARMA). The observations are consistent with each other and show inferred magnetic field lines aligned with the outflow. The CARMA observations suggest a full hourglass magnetic field morphology centered about the core; this is only the second well-defined hourglass detected around a low-mass protostar to date. We apply two different methods to CARMA polarimetric observations to estimate the plane-of-sky magnetic field magnitude, finding values of 1.4 and 3.4 mG.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.