A study of the far infrared counterparts of new candidates for planetary nebulae

Details A study of the far infrared counterparts of new candidates for planetary nebulae A study of the far infrared counterparts of new candidates for planetary nebulae

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.122..257i&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 122, no. 2, May 1986, p. 257-262.

Astronomy and Astrophysics

Astronomy

1

Brightness Distribution, Far Infrared Radiation, Planetary Nebulae, Surface Properties, Astronomical Catalogs, Chemical Evolution, Galactic Evolution, Infrared Astronomy Satellite, Interstellar Gas, Point Sources

Scientific paper

The IRAS Point Source Catalog was searched for infrared counterparts of the fourteen new candidates for planetary nebulae of low surface brightness detected by Hartl and Tritton (1985). Five of these candidates were identified with sources in the Catalog. All five nebulae are found in regions of high cirrus flux at 100 microns, and all have both point sources and small size extended sources with numbers varying from field to field. The infrared emission from these nebulae is connected with dust temperatures of about 100 K, characteristic of planetary nebulae.

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