Properties of the Variation of the Infrared Emission of Oh/ir Stars II. The L Band Light Curves

Details Properties of the Variation of the Infrared Emission of Oh/ir Stars II. The L Band Light Curves Properties of the Variation of the Infrared Emission of Oh/ir Stars II. The L Band Light Curves

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jkas...43..123k&link_type=abstract

Journal of the Korean Astronomical Society, vol. 43, no. 4, pp. 123-133

Astronomy and Astrophysics

Astronomy

Stars, Agb And Post-Agb, Infrared: Stars, Stars: Oscillations, Circumstellar Matter, Dust, Extinction

Scientific paper

In order to study properties of the pulsation in the infrared emission for long period variables, we collect and analyze the infrared observational data at L band for 12 OH/IR. The observation data cover about three decades including recent data from the ISO and Spitzer. We use the Marquardt-Levenberg algorithm to determine the pulsation period and amplitude for each star and compare them with results of previous investigations at infrared and radio bands. We obtain the relationship between the pulsation periods and the amplitudes at L band. Contrary to the results at K band, there is no difference of the trends in the short and long period regions of the period-luminosity relation at L band. This may be due to the molecular absorption effect at K band. The correlations among the L band parameters, IRAS [12-25] colors, and K band parameters may be explained as results of the dust shell parameters affected by the stellar pulsation. The large scatter of the correlation could be due to the existence of a distribution of central stars with various masses and pulsation modes.

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