Abstract
U, B, andV observations of AR Lacertae, obtained in 1981, have been presented alongwith the colour indices. A distortion wave minimum is found to lie at 0 P. 21. The amplitude of the wave minimum inV filter is too weak, while it is stronger inU andV filters, the strongest being inV filter. The period of the migration wave turns out to be 2.53 yr.
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Srivastava, R. K.: 1986, in press.
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Srivastava, R.K. Wave minimum of AR Lacertae. Astrophys Space Sci 121, 397–401 (1986). https://doi.org/10.1007/BF00653710
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DOI: https://doi.org/10.1007/BF00653710