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HD 205705

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The Spacelab-1 Very Wide Field Survey of UV-excess objects. IV. The performance of the instrument in combination with optical photometry as a means of identifying stars with peculiar properties. UV (195 nm) and Stroemgren uvby photometry of a 110 square degree fieldat high southern galactic latitudes are analyzed through a comparison ofi) UV magnitudes for 57 stars of various types common to the publishedTD1 catalogue and the Very Wide Field Camera (VWFC); and ii) observedand theoretical two-colour diagrams. The higher sensitivity of the VWFC(=~0.5magnitude) and its more complete survey are exemplified by thedetection and UV measurement of a series of objects with moderateUV-excess in addition to detection of some very blue objects of variousnature down to fainter than 12th magnitude in the optical domain. Adeeper survey with a VWFC-type instrument could provide a completesample for studies of the group properties of faint blue stars. Duringthe uvby reductions it was found that the usual procedure of plottingresiduals as functions of declination, hour angle and airmass can be apowerful and diagnostic test of photometer rigidity.
A Search for Beta-Cephei Type Variability in a Sample of Intermediate Galactic Latitude to High Galactic Latitude B-Type Stars Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1994MNRAS.267.1103H&db_key=AST
The galactic reddening law - The evidence from uvby-beta photometry of B stars Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1985A&A...142..189T&db_key=AST
Four-colour and H beta photometry of southern B stars at high galactic latitudes Four-color and H beta photometry has been obtained for 105 early-type HDstars with galactic latitudes less than -45 deg. They are mostly late Bstars of luminosity class V to III. Two new Am stars and several Ap orBp stars are detected photometrically. Absolute magnitudes aredetermined from the photometry and from MK types where available. Theinterstellar reddening of many of the more distant stars is very small,suggesting either the existence of undetected peculiar stars in thesample or that there are areas of effectively zero reddening at highsouthern galactic latitudes.
Photometry of silicon stars. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1977A&A....54..443H&db_key=AST
Faint blue stars in the region near the South Galactic Pole. Not Available

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Osservazione e dati astrometrici

Costellazione:	Capricorno
Ascensione retta:	21^h37^m37.67^s
Declinazione:	-19Â°13'51.7"
Magnitudine apparente:	7.434
Distanza:	201.613 parsec
Moto proprio RA:	13.2
Moto proprio Dec:	-0.5
B-T magnitude:	7.343
V-T magnitude:	7.427

Cataloghi e designazioni:

Nomi esatti	(Edit)
HD 1989	HD 205705
TYCHO-2 2000	TYC 6370-918-1
USNO-A2.0	USNO-A2 0675-36534959
HIP	HIP 106768

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