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HD 942


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Accurate Positions Of Suspected Variable Stars Near The South Galactic Pole
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Near-infrared photometry of stars
Results are presented of infrared photometric observations performed oncomparison stars during a monitoring of long-period variables. Theseobservations, spread over a lapse of about 5 years, are used to derivethe J, H, and K magnitudes of 54 stars in the photometric systemdescribed by Koornneef (1983). The 1950.0 coordinates, spectral types,visual magnitudes, average magnitudes, and the number of observationsare given for each object.

The Identification of IRAS Point Sources - Part One - a 304-DEGREE Field Centred on the South Galactic Pole
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1986MNRAS.223..279W&db_key=AST

E. W. Fick Observatory stellar radial velocity measurements. I - 1976-1984
Stellar radial velocity observations made with the large vacuumhigh-dispersion photoelectric radial velocity spectrometer at FickObservatory are reported. This includes nearly 2000 late-type starsobserved during 585 nights. Gradual modifications to this instrumentover its first eight years of operation have reduced the observationalerror for high-quality dip observations to + or - 0.8 km/s.

Radial velocities of southern stars obtained with the photoelectric scanner CORAVEL. III - 790 late-type bright stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1985A&AS...59...15A&db_key=AST

Radial velocities of southern HR stars
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1980PASP...92..713B&db_key=AST

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Datos observacionales y astrométricos

Constelación:Escultor
Ascensión Recta:00h13m42.10s
Declinación:-26°01'19.0"
Magnitud Aparente:5.94
Distancia:310.559 parsecs
Movimiento Propio en Ascensión Recta:39.5
Movimiento Propio en Declinación:-76.4
B-T magnitude:7.969
V-T magnitude:6.122

Catálogos y designaciones:
Nombres Propios   (Edit)
HD 1989HD 942
TYCHO-2 2000TYC 6416-1019-1
USNO-A2.0USNO-A2 0600-00094236
BSC 1991HR 42
HIPHIP 1096

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