THE CIRCUMSTELLAR SHELLS OF CARBON MIRAS

Authors
Citation
M. Groenewegen, THE CIRCUMSTELLAR SHELLS OF CARBON MIRAS, Astrophysics and space science, 224(1-2), 1995, pp. 321-324
Citations number
14
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
0004640X
Volume
224
Issue
1-2
Year of publication
1995
Pages
321 - 324
Database
ISI
SICI code
0004-640X(1995)224:1-2<321:TCSOCM>2.0.ZU;2-7
Abstract
The relation between mass loss rate and pulsation period in carbon Mir as is discussed. The dust mass loss rate is very low (about 2 x 10(-10 ) M./yr) up to about P = 380 days, where there is a sudden increase. F or P > 400 days there is a linear relation between log M and P. The ch ange in the mass loss rate near 380 days may be related to radiation p ressure on dust becoming effective in driving the outflow.