Some of What 1612 MHz Masers Tell Us about the dM/dt of OH/IR Stars

Details Some of What 1612 MHz Masers Tell Us about the dM/dt of OH/IR Stars Some of What 1612 MHz Masers Tell Us about the dM/dt of OH/IR Stars

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..311l&link_type=abstract

Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes. ASP Conference Series, Vol. 378, proceedings of the co

Astronomy and Astrophysics

Astronomy

Scientific paper

80% of the most massive OH/IR stars with the reddest mid-infrared colors appear to have detached shells: these are due to a strongly modulated mass-loss rate on a much longer time-scale than their pulsational periods. The complete switching OFF & ON of 1612 MHz masers in the low-mass star IRAS 19479+2111 suggests now that all OH/IR stars have a strongly modulated dM/dt.

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