A Long-Term Study of Pulsational Light Variability in Post--AGB Stars

Details A Long-Term Study of Pulsational Light Variability in Post--AGB Stars A Long-Term Study of Pulsational Light Variability in Post--AGB Stars

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..303h&link_type=abstract

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

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3

Scientific paper

We have monitored 24 post--AGB stars for light variations. Periods are
determined for eight of these, ranging from 44 to 140 days, with
quasi-periods found in several others.

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