Mathematical analysis of some photometric peculiarities of AU Monocerotis

Details Mathematical analysis of some photometric peculiarities of AU Monocerotis Mathematical analysis of some photometric peculiarities of AU Monocerotis

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....85..342l&link_type=abstract

Astronomy and Astrophysics, vol. 85, no. 3, May 1980, p. 342-349.

Computer Science

Numerical Analysis

12

Astronomical Photometry, Eclipsing Binary Stars, Numerical Analysis, Variable Stars, Light Curve, Stellar Luminosity, Tables (Data)

Scientific paper

An analysis of photometric observations of AU Monocerotis, represented by 183 weighted normal points, has revealed a peculiarity of the light curve which is associated with the overlapping of two periodic phenomena: the well-known eclipsing one and a newly detected phenomenon with the provisional ephemeris Max(E) = 2443105 + 411 E. A tridimensional matrix representation is used to analyze the intrinsic luminosity variation of the system. A revision of the period using modified weights has yielded: M(E) = 2442801.375 + 11.113037 E.

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