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Photoelectric observations of the long-period eclipsing binaries at Yonsei University Observatory

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Photoelectric observations of the long-period eclipsing binaries at Yonsei University Observatory

by
Nha, I. S.; Lee, Y. S.; Chun, Y. W.; Kim, H. I.; Kim, Y. S

Publication date
Usage
Public DomainCreative Commons Licensepublicdomain
Topics
AURIGA CONSTELLATION, STOKES LAW OF RADIATION, VARIABLE STARS, VISUAL OBSERVATION, COLOR, ECLIPSING BINARY STARS, LIGHT CURVE, OPTICAL POLARIZATION, BRIGHTNESS, IUE, PULSED RADIATION, SPACE OBSERVATIONS (FROM EARTH)
Collection
nasa_techdocs
Contributor
NASA
Language
English
Rights
Public Domain
A long term project (ten-years; 1982-92) for the photoelectric observation in the UBV passbands of selected eclipsing binaries with P 10 days has initiated at Yonsei University Observatory using 40-cm and 61-cm reflectors. The instrumentation used and the observation techniques and the reduction procedures applied to this investigation are described.
Addeddate
2010-07-21 10:43:51
Documentid
19860002717
Identifier
nasa_techdoc_19860002717
Identifier-ark
ark:/13960/t3dz1045k
Ocr
ABBYY FineReader 8.0
Ppi
300
Year
1985

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