A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf.
Photoelectric photometry of GG Carinae
1983
Publications of the Astronomical Society of the Pacific
Preserved Fulltext
U, B, V, R, and I magnitudes of GG Car were determined in 1979. Variation of brightness was observed in an interval of 13 days. Its energy distribution was determined according to these and the published H, K, and L magnitudes. A model which consists of two stars of effective temperatures of 15,000 K and 4800 K and a circumstellar electron cloud is considered.
doi:10.1086/131138
fatcat:nc5sub6osrgeravwaxjixob7mu