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An HI 21-cm line survey of evolved stars
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The HI line at 21 cm is a tracer of circumstellar matter around AGB stars, and especially of the matter located at large distances (0.1-1 pc) from the central stars. It can give unique information on the kinematics and on the physical conditions in the outer parts of circumstellar shells and in the regions where stellar matter is injected into the interstellar medium. However this tracer has not been much used up to now, due to the difficulty of separating the genuine circumstellar emission from the interstellar one. With the Nancay Radiotelescope we are carrying out a survey of the HI emission in a large sample of evolved stars. We report on recent progresses of this long term programme, with emphasis on S-type stars.
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Cited by 1 Pith paper
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HI envelope around the carbon star V420 Vul
An extended ~20 pc HI structure around the carbon-rich Mira V420 Vul shows symmetric kinematics centered on the star, interpreted as a stellar wind imprint on a porous interstellar cloud.
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