Photoelectric photometry of the nova-like eclipsing variable PG1030+590

Details Photoelectric photometry of the nova-like eclipsing variable PG1030+590 Photoelectric photometry of the nova-like eclipsing variable PG1030+590

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cha%26a..13....2z&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 13, March 1989, p. 2-8. Translation.

Astronomy and Astrophysics

Astrophysics

Accretion Disks, Astronomical Photometry, Cataclysmic Variables, Eclipsing Binary Stars, Light Curve, Electrophotometry, Late Stars, Stellar Mass, White Dwarf Stars

Scientific paper

PG1030+590 is a recently discovered nova-like eclipsing variable. Results of high-speed photoelectric photometry and UBVR light curves are presented. Using the model of cataclysmic variables, it is found its geometrical and physical parameters to be as follows: mass of the white dwarf component = 0.83 + or - 0.22 solar masses, radius of the late-type component = 0.35 + or - 0.06 solar masses, and orbital inclination = 81 + or - 2 deg.

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