Photometric Investigation of the Eclipsing Binary Star KN Per

Details Photometric Investigation of the Eclipsing Binary Star KN Per Photometric Investigation of the Eclipsing Binary Star KN Per

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.254..295g&link_type=abstract

Astrophysics and Space Science, v. 254, Issue 2, p. 295-304 (1997).

Astronomy and Astrophysics

Astrophysics

5

Scientific paper

We used the Behlen observatory 0.76 m telescope and the CCD photometer to secure 689 observation of the eclipsing binary star KN Per. The observations were made on 8 nights during 1993 and 1994 with V and R bandpass filters. From 7 determinations of eclipse timings of minimum (V&R together), we have determined a new epoch and an orbital period of 0.8664604 days. The published spectral classification is A9.

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