Small-Amplitude Red Variables in the AAVSO Photoelectric Program: Light Curves and Periods

Small-amplitude red variables (SARVs) are M giants or supergiants which are pulsating with small amplitudes (up to 2.5 mag) and with time scales of 20-200 days or more. This paper reports on a 10-yr study of about two dozen SARVs, carried out through the American Association of Variable Star Observe...

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Veröffentlicht in:Publications of the Astronomical Society of the Pacific 1996-02, Vol.108 (720), p.139-145
Hauptverfasser: Percy, John R., Desjardins, Adrien, Yu, Lawrence, Landis, Howard J.
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creator Percy, John R.
Desjardins, Adrien
Yu, Lawrence
Landis, Howard J.
description Small-amplitude red variables (SARVs) are M giants or supergiants which are pulsating with small amplitudes (up to 2.5 mag) and with time scales of 20-200 days or more. This paper reports on a 10-yr study of about two dozen SARVs, carried out through the American Association of Variable Star Observers (AAVSO) photoelectric photometry program. It has provided detailed information on the regularity, period, and amplitude of these stars. Most have well-defined periods in the 20-200 day range.Several also have a long secondary period. One (W Boo) appears to have two periods with a ratio of 2.3.
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source Jstor Complete Legacy; Institute of Physics Journals; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection
subjects Astronomical magnitude
Astronomical photometry
Autocorrelation
Light curves
Mathematical minima
Stars
Supergiant stars
Variable stars
Visible spectrum
Weak minimum
title Small-Amplitude Red Variables in the AAVSO Photoelectric Program: Light Curves and Periods
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