FBS 2213+421: A dust-enshrouded long-period AGB Mira variable?

Details FBS 2213+421: A dust-enshrouded long-period AGB Mira variable? FBS 2213+421: A dust-enshrouded long-period AGB Mira variable?

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap.....49...78g&link_type=abstract

Astrophysics, Volume 49, Issue 1, pp.78-82

Astronomy and Astrophysics

Astrophysics

Stars, Mira Type-Stars, Individual, Fbs 2213+421

Scientific paper

Very red optical and IR-color indices indicate the presence of a dense circumstellar shell around object FBS 2213+421. The estimated total mass-loss rate is typical for dust-enshrouded oxygen-rich Asymptotic Giant Branch (AGB) Long-Period Mira-type variables. K-band monitoring is necessary to determine the pulsation period, the absolute bolometric luminosity, and the distance to this object.

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