Observation of Interstellar Magnetic Field in a Dense Molecular Core with CCS Zeeman Effect

Details Observation of Interstellar Magnetic Field in a Dense Molecular Core with CCS Zeeman Effect Observation of Interstellar Magnetic Field in a Dense Molecular Core with CCS Zeeman Effect

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000asthe..93..361s&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 93, No. 7, p. 361 - 368 (2000)

Astronomy and Astrophysics

Astronomy

Scientific paper

The authors made CCS Zeeman observations toward a dense molecular cloud core in Taurus Molecular Cloud (TMC), L1521E, by using a new polarimeter system developed for the Nobryama 45-m telescope. The polarimeter system covers a wide millimeter-wavelength range (1.2 - 8.6mm). They confirmed their calculation values for the low-N rotational state of Zeeman effect of CCS. The measured value of the magnetic field strength was 160 ± 42 microgauss, which suggests that the core is in magnetically subcritical state.

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