The 1.3 MM continuum emission from circumstellar envelopes

Details The 1.3 MM continuum emission from circumstellar envelopes The 1.3 MM continuum emission from circumstellar envelopes

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990liaco..29..155w&link_type=abstract

In ESA, From Ground-Based to Space-Borne Sub-mm Astronomy p 155-157 (SEE N91-21986 13-89)

Astronomy and Astrophysics

Astronomy

Continuum Flow, Emission Spectra, Millimeter Waves, Mira Variables, Stellar Radiation, Infrared Astronomy, Line Spectra, Spectrum Analysis, Stellar Envelopes, Stellar Oscillations

Scientific paper

Results of a survey carried out on the 1.3 mm continuum emission, from
the circumstellar envelopes of late type stars are presented. Some 26
out of 38 stars are detected including several Mira variables and OH-IR
stars. It is concluded that the emission from the optically visible Mira
variables and semiregulars is photospheric in origin.

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