The Circumstellar Shells of Carbon Miras

Details The Circumstellar Shells of Carbon Miras The Circumstellar Shells of Carbon Miras

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..321g&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 321-324

Astronomy and Astrophysics

Astrophysics

5

Agb Stars, Mass Loss, Long Period Variables

Scientific paper

The relation between mass loss rate and pulsation period in carbon Miras is discussed. The dust mass loss rate is very low (about 2 × 10-10 M&sun;/yr) up to aboutP = 380 days, where there is a sudden increase. ForP > 400 days there is a linear relation between logM andP. The change in the mass loss rate near 380 days may be related to radiation pressure on dust becoming effective in driving the outflow.

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