Planetary nebulae near the galactic center. I - Method of discovery and preliminary results

Details Planetary nebulae near the galactic center. I - Method of discovery and preliminary results Planetary nebulae near the galactic center. I - Method of discovery and preliminary results

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...205..248p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 205, no. 1-2, Oct. 1988, p. 248-256.

Astronomy and Astrophysics

Astronomy

125

Far Infrared Radiation, Galactic Nuclei, Milky Way Galaxy, Planetary Nebulae, Radio Sources (Astronomy), Infrared Astronomy Satellite, Luminosity, Radiant Flux Density, Spatial Distribution, Very Large Array (Vla)

Scientific paper

A method is described for finding planetary nebulae (PN). Use is made of the far infrared IRAS colors and radio continuum measurements. The method is applied here to a region within 15° of the galactic center. The first results are given, including 36 new PN. The characteristics of the nebulae are described. While they are generally similar to known nebulae, the method of selection gives an emphasis to younger objects. A substantial number of the new nebulae may be in the transition phase between OH/IR stars and PN.

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