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Walraven VBLUW photometry in Basel halo fields. I - Photometric data for selected areas SA141 (South Galactic Pole), SA94 and SA107 In 1981 a joint Swiss-Dutch program was initated to obtain photoelectricphotometry in the Walraven VBLUW system for F-G stars in fields of theBasel halo survey. The aim of this project is to determine temperature,surface gravity, and metal abundance for these stars in order to studythe distribution of the average stellar metallicity as a function ofdistance from the galactic place up to z-distances of about 1 kpc. Thispaper presents the VBLUW data for 112 program stars in Selected AreaSA141 at the South Galactic Pole, 93 stars in SA94 (l = 175 deg, b = -49deg), and 46 stars in SA107 (l = 6 deg, b = +41 deg).
| A survey of trigonometric parallaxes and proper motions with the UK Schmidt telescope. II - Astrometric and photometric data for a complete sample of 6125 stars brighter than B = 17.5, V = 17.0 in the South Galactic CAP Abstract image available at:http://adsabs.harvard.edu/abs/1986MNRAS.223..629M
| Interstellar polarization from observations of A and F stars in high and intermediate galactic latitudes, and from stars in the Mathewson and Ford polarization catalogue Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1986A&AS...64..487K&db_key=AST
| Stellar Distribution Near the South Galactic Pole, Photographic V Magnitudes and (B-V) Colours of 640 Stars in Region I. Not Available
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Gözlemler ve gökölçümü verileri
Takýmyýldýz: | Yontar |
Sað Açýklýk: | 01h04m29.94s |
Yükselim: | -29°47'48.7" |
Görünürdeki Parlaklýk: | 8.837 |
Uzaklýk: | 223.714 parsek |
özdevim Sað Açýklýk: | 26.8 |
özdevim Yükselim: | -12.6 |
B-T magnitude: | 9.393 |
V-T magnitude: | 8.883 |
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