Photometry of yellow semi-regular variables - WY And

Details Photometry of yellow semi-regular variables - WY And Photometry of yellow semi-regular variables - WY And

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.165..111z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 165, no. 1, March 1990, p. 111-118.

Astronomy and Astrophysics

Astrophysics

13

Astronomical Photometry, Semiregular Variable Stars, Electrophotometry, Mira Variables, Stellar Evolution, Stellar Magnitude, Stellar Oscillations

Scientific paper

WY And was observed photoelectrically in the years 1984-1988. Its period
is 109.65 days, though it is not constant. The variable is probably
pulsating in the fundamental mode. In spite of theoretical predictions,
the star does not show any sign of chaotic behavior.

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