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 mu m) 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.
| Original language | English |
|---|---|
| Article number | 15 |
| Number of pages | 6 |
| Journal | Astrophysical Journal Letters |
| Volume | 769 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 20-May-2013 |
Keywords
- galaxies: star formation
- magnetic fields
- polarization
- stars: protostars
- 350 MU-M
- STAR-FORMATION
- SUBMILLIMETER POLARIZATION
- MOLECULAR CLOUDS
- IRAS 4A
- CORES
- OUTFLOW
- DUST
- POLARIMETRY
- ENVELOPE
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