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HD 204187


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The S201 far-ultraviolet imaging survey. II - A field in Cygnus
Far-ultraviolet imagery of a region in Cygnus, a 20 deg diameter fieldcentered near (1950) R. A. 21 h 31.2 m decl. +37 deg 25 arcmin, wasobtained by the S201 far-ultraviolet camera during the Apollo 16mission. In a 10 minute exposure covering the 1250-1600 A wavelengthrange (effective wavelength 1400 A), 730 star images can be detected,corresponding to a limiting ultraviolet magnitude of about m (1400) =10. Assuming nominal interstellar extinction values in this region nearthe galactic plane, this result corresponds to the detection of A0 Vstars to a distance of 300 pc and of B0 V stars to 1500 pc.Uncertainties in spectral classification and interstellar extinction forindividual objects are probably more significant than calibration ormeasurement errors. Most of the objects detected are identified withstars in the Smithsonian Astrophysical Observatory Star Catalog (1966),or the Catalog of Stellar Identifications (1979) or both, but 87 objectsremain unidentified (or are identified with late-type stars).

Absolute Emission-Line Intensities in Planetary Nebulae. I.
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观测天体数据

星座:天鵝座
右阿森松:21h25m50.04s
赤纬:+38°30'58.4"
视星:8.497
距离:303.03 天文距离
右阿森松适当运动:-2.8
赤纬适当运动:2.7
B-T magnitude:8.66
V-T magnitude:8.511

目录:
适当名称   (Edit)
HD 1989HD 204187
TYCHO-2 2000TYC 3182-3642-1
USNO-A2.0USNO-A2 1275-15646004
HIPHIP 105817

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