Bipolar radio morphology in the compact nebula K3-35

Details Bipolar radio morphology in the compact nebula K3-35 Bipolar radio morphology in the compact nebula K3-35

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...222..227a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 222, no. 1-2, Sept. 1989, p. 227-230. Research supported by NSERC.

Astronomy and Astrophysics

Astronomy

14

Continuous Radiation, H Ii Regions, Morphology, Planetary Nebulae, Radio Sources (Astronomy), Emission Spectra, Hydroxyl Emission, Interstellar Masers, Line Spectra

Scientific paper

The observation of a highly bipolar radio morphology of the object K3-35 is reported, which has been suggested to be a young planetary nebula or a compact H II region. It is found that the infrared energy distribution of K3-35 is similar to that of other compact planetary nebulas, but that the observed radio structure shows an extreme bipolar form not seen in most planetary nebulas.

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