Circular and linear polarization of the SiO masers in VY Canis Majoris

Details Circular and linear polarization of the SiO masers in VY Canis Majoris Circular and linear polarization of the SiO masers in VY Canis Majoris

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...428l..29m&link_type=abstract

The Astrophysical Journal, vol. 428, no. 1, pt. 1, p. L29-L32

Astronomy and Astrophysics

Astronomy

11

Astronomical Photometry, Circular Polarization, Interstellar Masers, Linear Polarization, Stellar Envelopes, Radio Astronomy, Zeeman Effect

Scientific paper

The circular and linear polarization parameters of the SiO masers in VY
CMa have been measured in the v = 1, J = 2 - 1 (86 GHz) and v = 1, J = 1
- 0 (43 GHz) transitions. The higher frequency is less circularly
polarized than the lower frequency transition.

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