The light curve at 10 microns of Algol near secondary minimum

Details The light curve at 10 microns of Algol near secondary minimum The light curve at 10 microns of Algol near secondary minimum

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184..523n&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, Aug. 1978, p. 523-525.

Astronomy and Astrophysics

Astronomy

6

Algol, Infrared Astronomy, Light Curve, Variable Stars, Gravitational Effects, Stellar Magnitude

Scientific paper

Observations of Algol (Beta Persei) at 10 microns are presented which are of relevance to the system's behavior around the time of its secondary minimum. No evidence is found for a significant excess at 10 microns. The data show a smooth decline by 0.3 mag which starts at about phase 0.42, while the limited data obtained at phases greater than 0.50 are consistent with a symmetrical curve about phase 0.50.

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