A radio study of planetary nebulae

Details A radio study of planetary nebulae A radio study of planetary nebulae

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...234..387z&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 234, no. 1-2, Aug. 1990, p. 387-395. Research supported by NWO.

Astronomy and Astrophysics

Astronomy

17

Luminous Intensity, Planetary Nebulae, Radio Astronomy, Stellar Evolution, Flux Density, Very Large Array (Vla)

Scientific paper

Planetary nebulae in the Galactic bulge and elsewhere are studied using a large set of radio flux measurements. The distribution of flux densities as a function of diameter are compared with theoretical models and it is shown how the radio brightness temperature can be used to test the models. The mass-radius relation and how it influences planetary nebula evolution is discussed. The variation of the IR excess with position in the Galaxy is studied as well.

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