A reanalysis of the light curve of RT Persei with the W-D code

Details A reanalysis of the light curve of RT Persei with the W-D code A reanalysis of the light curve of RT Persei with the W-D code

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.243..275e&link_type=abstract

Astrophysics and Space Science, Volume 243, Issue 2, pp.275-283

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

The UBV photometric observations of RT Per, from Sanwal and Chaubey (1981), were analyzed by the Wilson and Devinney code (1971). The light curves include reflection effects that for the first time has been suggested by Dugan (1911). RT Per has a semi-detached configuration where the lower-mass component is in contact with its respective Roche surface. The higher-mass component very nearly fills its Roche lobe. It has the characteristic of an Algol type system. The absolute dimensions for the primary and secondary of this system were calculated from its spectral types and by combining the photometric solution with inferred component radial velocities (Lu, 1990).

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