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The magnetic field morphology of the class 0 protostar L1157-mm

  • Ian W. Stephens
  • , Leslie W. Looney
  • , Woojin Kwon
  • , Charles L.H. Hull
  • , Richard L. Plambeck
  • , Richard M. Crutcher
  • , Nicholas Chapman
  • , Giles Novak
  • , Jacqueline Davidson
  • , John E. Vaillancourt
  • , Hiroko Shinnaga
  • , Tristan Matthews

Research output: Contribution to journalArticlepeer-review

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 μm) 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 languageEnglish (US)
Article numberL15
JournalAstrophysical Journal Letters
Volume769
Issue number1
DOIs
StatePublished - May 20 2013

Keywords

  • galaxies: star formation
  • magnetic fields
  • polarization
  • stars: protostars

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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