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HD 118256


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UVBY H-beta photometry of UV-bright stars
uvby H-beta photometry is presented for 90 stars taken from an earlyversion of the Carnochan and Wilson (1983) catalogue of stars that havevery negative UV colors. Two have definite UV excesses (HD 36629, and HD81307). Four early-B stars have UV colors too positive for their visibleclassification, and beta-indices that indicate higher luminosities thanappear possible on galactic distribution grounds. Six late-B starsappear to have discordant flux distributions for which there are noobvious explanations. It is suggested that the high population ofsubluminous stars derived by Carnochan and Wilson is the product of thestatistical treatment used and the extreme patchiness in theinterstellar absorption, which gives rise to large numbers oflittle-reddened stars.

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Gözlemler ve gökölçümü verileri

Takýmyýldýz:Erbogan
Sað Açýklýk:13h36m43.55s
Yükselim:-53°11'29.4"
Görünürdeki Parlaklýk:8.013
Uzaklýk:320.513 parsek
özdevim Sað Açýklýk:-6.5
özdevim Yükselim:-4
B-T magnitude:7.928
V-T magnitude:8.006

Kataloglar ve belirtme:
Özgün isimleri
HD 1989HD 118256
TYCHO-2 2000TYC 8663-1387-1
USNO-A2.0USNO-A2 0300-18930639
HIPHIP 66390

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