Circumstellar Absorption and Emission in the Post-AGB Stars HR4049 and HD213985

Details Circumstellar Absorption and Emission in the Post-AGB Stars HR4049 and HD213985 Circumstellar Absorption and Emission in the Post-AGB Stars HR4049 and HD213985

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..357w&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 357-360

Astronomy and Astrophysics

Astrophysics

7

Post-Agb Stars, Circumstellar Matter, Hr 4049, Hd 213985

Scientific paper

The evolved C-rich low-mass stars HR 4049 and HD 213985 present variable
circumstellar extinction and emission. Observations of HR 4049
strengthen the link between the far-UV extinction rise and the presence
of small C-rich particles. Variability of the UV absorption bump in HD
213985 is reported here for the first time and is discussed.

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