Mass loss history of the local Miras

Details Mass loss history of the local Miras Mass loss history of the local Miras

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..219n&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Miras, Iras, Period, Mass Loss

Scientific paper

Mira variables in the solar neighbourhood were selected from the IRAS
Point Source Catalog with the help of the period-luminosity relation.
The distribution of the IRAS color log(F25/F12) changes abruptly when
the period exceeds 290 days. The implication of this changes is
discussed.

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