Astron. Astrophys. Suppl. Ser. 130, 1-64
R. Neri1, C. Kahane2, R. Lucas1, V. Bujarrabal3, and C. Loup4
Send offprint request: R. Neri
1 - IRAM, 300 rue de la Piscine, 38406 S Martin
d'Hères, France
2 - Observatoire de Grenoble, BP. 53, 38041 Grenoble
Cedex 9, France
3 - Observatorio Astronómico Nacional (I.G.N),
Apartado 1143, 28800 Alcalá de Henares, Madrid, Spain
4 - Institut d'Astrophysique de Paris, CNRS, 98 bis Bd. Arago, 75014 Paris,
France
Received June 30; accepted October 28, 1997
We present the results of a 12CO() and (
) survey on a sample of 46
objects classified as AGB and post-AGB stars. We have obtained fully
sampled high resolution maps of their 12CO(
) emission by combining
visibilities from the IRAM interferometer with short spacing
observations from the IRAM 30 m telescope. Properties of their
circumstellar envelopes like fluxes, radii, and positions are derived
from model fits to the visibilities and compared to the results
obtained from 12CO(
) maps observed at the IRAM 30 m telescope. From the
12CO(
) observations we have derived mass loss rates for 38 stars and
established an empirical relation between the CO photodissociation
radius of an envelope and the measured radius in the (
) emission.
Key words: Atlases -- stars: AGB, post-AGB -- stars: circumstellar matter -- stars: mass-loss -- stars: evolution -- radio lines: stars
Copyright The European Southern Observatory (ESO)