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HD 147181


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Artículos relacionados

Far-Ultraviolet Stellar Photometry: Fields Centered on rho Ophiuchi and the Galactic Center
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1996ApJS..104..101S&db_key=AST

Far-ultraviolet stellar photometry: Fields in Sagittarius and Scorpius
Far-ultraviolet photometry for 741 objects in a field in Sagittariuscentered near M8 and 541 objects in a field centered near sigma Scorpiiis presented. These data were extracted from electographic imagesobtained with two cameras during a shuttle flight in 1991 April/May. Thecameras provided band passes with lambdaeff = 1375 A andlambdaeff = 1781 A. Synthetic colors show that these bandsare sensitive to effective temperature for hot stars. Our measurementswere placed on a quantitative far-ultraviolet magnitude scale byconvolving the spectra of stars observed by IUE with our cameras'spectral response functions. Fifty-eight percent of the ultravioletobjects were identified with visible stars using the SIMBAD databasewhile another 40% of the objects are blends of early type stars tooclose together to separate with our resolution. Our photometry iscompared with that from the TD-1, OAO 2, and ANS satellites and the S201(Apollo 16) far-ultraviolet camera and found to agree at the level of afew tenths of a magnitude. Unlike previous studies, almost half of theidentified visual counterparts to the ultraviolet objects are early Bstars. A plot of distance modulus against ultraviolet color excessreveals a significant population of stars with strong ultravioletexcess.

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Datos observacionales y astrométricos

Constelación:Regla
Ascensión Recta:16h22m14.39s
Declinación:-43°12'00.9"
Magnitud Aparente:7.622
Distancia:157.729 parsecs
Movimiento Propio en Ascensión Recta:5.7
Movimiento Propio en Declinación:-18
B-T magnitude:7.813
V-T magnitude:7.638

Catálogos y designaciones:
Nombres Propios
HD 1989HD 147181
TYCHO-2 2000TYC 7865-2295-1
USNO-A2.0USNO-A2 0450-23953452
HIPHIP 80186

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