Spectral Variations in Fading Episodes of Carbon Stars

Details Spectral Variations in Fading Episodes of Carbon Stars Spectral Variations in Fading Episodes of Carbon Stars

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..313l&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

1

Scientific paper

The J--type carbon star T Mus undergoes fadings at intervals of about three years, during which emission appears in the C2 bands and the strength and structure of the SiC2 bands change. The appearance of similar emission features in the C2 bands of carbon Miras suggests a connection between the fundamental-mode pulsations of the latter and the slow variations of T Mus, which is a semiregular variable.

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