The Unique Eclipsing System KH 15D: Photometry

Details The Unique Eclipsing System KH 15D: Photometry The Unique Eclipsing System KH 15D: Photometry

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..349..189b&link_type=abstract

Astrophysics of Variable Stars, Pecs, Hungary, 5-10 September 2005, Sterken, C. and Aerts, C. (eds). ASP Conference Series, Vol.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present results of photometric observations of the young eclipsing binary KH 15D obtained during three observing seasons of 2002--2005. A comparison of our data with data from the literature reveals the existence of the long-term photometrical brightness trend: during 4.5 years a system brightness in the Ic-band decreased by about one stellar magnitude.

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