Light variations of 28 Andromedae

Details Light variations of 28 Andromedae Light variations of 28 Andromedae

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...144..211g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 144, no. 1, March 1985, p. 211-214.

Astronomy and Astrophysics

Astrophysics

9

Annual Variations, Light Curve, Spectral Energy Distribution, Spectrum Analysis, Variable Stars, Ephemerides, Fourier Transformation

Scientific paper

Analysis of existing and new photometric observations of the δ
Scuti type star 28 Andromedae indicates that it is a monoperiodic
variable star with a period of 0d.0693 with notable amplitude
variations from season to season. Evidence presented suggests that 28
And is a second overtone pulsator.

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