The features of infra-red emission of planetary nebulae in the inner galaxy

Details The features of infra-red emission of planetary nebulae in the inner galaxy The features of infra-red emission of planetary nebulae in the inner galaxy

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.219..117a&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 219, no. 1, p. 117-134

Astronomy and Astrophysics

Astronomy

3

Infrared Astronomy, Infrared Radiation, Infrared Sources (Astronomy), Milky Way Galaxy, Planetary Nebulae, Classifications, Correlation, Distance, Spatial Distribution

Scientific paper

414 galactic planetary nebulae (PN) with measured infra-red luminosities (302 of which are located within the sector of galactic longitudes from 345 deg to 15 deg) are investigated. All nebulae are subdivided into four mass classes and different distance scales for each class are used. Planetary nebulae located in the inner Galaxy are selected. The galactic radial gradients of infra-red luminosities and excesses are obtained for each nebula mass class. Possible explanations of the effect are discussed.

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