An infrared sequence in the late stages of stellar evolution

Details An infrared sequence in the late stages of stellar evolution An infrared sequence in the late stages of stellar evolution

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.244..179k&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 244, May 1, 1990, p. 179-183.

Astronomy and Astrophysics

Astronomy

23

Infrared Sources (Astronomy), Late Stars, Stellar Evolution, Absorption Spectra, Asymptotic Giant Branch Stars, Color-Color Diagram, Emission Spectra, Infrared Astronomy Satellite, Planetary Nebulae

Scientific paper

Late-type stars showing the 9.7-micron feature in emission or absorption are found to occupy different parts of the color-color diagram. Furthermore, these objects are separated in color from planetary nebulae which have high radio surface brightness. The color distribution of these classes of objects suggests the presence of a continuous infrared sequence, connecting the asymptotic giant branch and planetary nebulae phases, which allows for the search for transitional objects between these two evolutionary phases.

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