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HD 179152


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Stroemgren photometry of F- and G-type stars brighter than V = 9.6. I. UVBY photometry
Within the framework of a large photometric observing program, designedto investigate the Galaxy's structure and evolution, Hβ photometryis being made for about 9000 stars. As a by-product, supplementary uvbyphotometry has been made. The results are presented in a cataloguecontaining 6924 uvby observations of 6190 stars, all south ofδ=+38deg. The overall internal rms errors of one observation(transformed to the standard system) of a program star in the interval6.5

Note on the nature of HD 179315
MK classification and UBVRI photometry is carried out to determinewhether the HD 179315 star is a cepheid or an ellipsoidal binary. Thespectral type proved to be G1Ib, classifying the star as a seven-daycepheid. This is supported by UBVRI data, from which is derived E(B-V) =0.48 plus or minus 0.03 on the Parsons-Bell color excess scale. The staris distinctly cooler than most seven-day cepheids, and is probably closeto the red edge of the instability strip, which may account for its lowamplitude of 0.3 magnitudes.

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观测天体数据

星座:天鷹座
右阿森松:19h11m15.37s
赤纬:+04°11'27.9"
视星:7.488
距离:118.343 天文距离
右阿森松适当运动:16.6
赤纬适当运动:-7.2
B-T magnitude:8.347
V-T magnitude:7.559

目录:
适当名称
HD 1989HD 179152
TYCHO-2 2000TYC 471-2351-1
USNO-A2.0USNO-A2 0900-14115420
HIPHIP 94268

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