The nature of the GN20.18.3 nebulosity

Details The nature of the GN20.18.3 nebulosity The nature of the GN20.18.3 nebulosity

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.250..111s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 250, May 1, 1991, p. 111-114. SERC-supported research.

Astronomy and Astrophysics

Astronomy

3

Emission Spectra, Herbig-Haro Objects, Reflection Nebulae, Stellar Envelopes, Cygnus Constellation, Dark Matter, Polarized Electromagnetic Radiation, Stellar Winds

Scientific paper

GN20.18.3 is a bipolar reflection nebula illuminated by a central star
which is surrounded by an extensive circumstellar disk at position angle
125 deg. The associated Herbig-Haro object is a knot-like concentration
of gas and dust and is seen in both scattered light and shock excited
intrinsic emission.

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