A polarization study of the cometary nebula Parsamyan 21

Details A polarization study of the cometary nebula Parsamyan 21 A polarization study of the cometary nebula Parsamyan 21

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.212p...1d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 212, Jan. 1, 1985, p. 1P-4P. Research supported by the

Astronomy and Astrophysics

Astronomy

23

Cometary Atmospheres, Polarimetry, Reflection Nebulae, Linear Polarization, Polarization Characteristics, Stellar Envelopes

Scientific paper

Polarization data are presented for the cometary nebula Parsamyan 21. The nebula is a relatively highly polarized and illuminated by the apical star within it. Across the head of the nebula and including the illuminating star is a band of polarization which may be due to aligned grains in a circumstellar torus. Parsamyan 21 is very similar in polarization structure to the well-studied cometary nebulae NGC 2261 and 6729, illuminated by R Mon and R CrA respectively.

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