Interpretation of Orbital Light Curves of U Geminorum

Details Interpretation of Orbital Light Curves of U Geminorum Interpretation of Orbital Light Curves of U Geminorum

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003arep...47..848k&link_type=abstract

Astronomy Reports, vol. 47, Issue 10, p.848-864

Astronomy and Astrophysics

Astronomy

2

Scientific paper

We interpret optical and IR orbital light curves of the dwarf nova U Gem in its quiescent state in the framework of “hot line” and “hot spot” models. The hot-line model provides an adequate fit to the light curves, while the hot-spot model is not fully consistent with the observations. The minimum χ2 residuals for the hot-spot and hot-line models are 2203 and 168, respectively.

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