The photometric variations of the AP star HD34631

Details The photometric variations of the AP star HD34631 The photometric variations of the AP star HD34631

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26as...90...19m&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 90, no. 1, Oct. 1991, p. 19-23.

Astronomy and Astrophysics

Astrophysics

6

A Stars, Peculiar Stars, Periodic Variations, Stellar Spectrophotometry, Light Curve, Stellar Color, Ultraviolet Photometry, Visual Photometry

Scientific paper

The photometric behavior in the uvby system of the Ap star HD34631 has
been reanalyzed on the basis of data collected over a time span of 16
years. A more accurate value of the period is deduced: P = 2.20269
+/-0.00004d. The lightcurves show a double-wave shape. The variations
are smallest in the v band.

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