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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
  • *Corresponding author for this work

    Research output: Contribution to journalArticleAcademicpeer-review

    98 Citations (Scopus)
    343 Downloads (Pure)

    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 languageEnglish
    Article number15
    Number of pages6
    JournalAstrophysical Journal Letters
    Volume769
    Issue number1
    DOIs
    Publication statusPublished - 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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