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Far-ultraviolet stellar photometry - A field in Monoceros
FUV photometry of stars in a field in Monoceros in the wavelength rangefrom 1230 to 1600 A has been carried out using data from anelectrographic Schmidt camera carried on a sounding rocket. Ultravioletmagnitudes were extracted for 602 objects in the field. Fifty-eightpercent were tentatively identified with visible stars using the SIMBADdata base while another 25 percent are blends of objects too closetogether to separate with our resolution. Eleven of the UV objectscoincide with parts of the star clusters NGC 2169, NGC 2244, and NGC2264 in which individual stars cannot be resolved. As in previousstudies, the majority of the identified ultraviolet sources areidentified with early-stars. However, there are a significant number forwhich no such identification was possible, and we suggest that many ofthese are nearby white dwarfs.
| Radial-velocity measurements. V - Ground support of the HIPPARCOS satellite observation program
The paper presents data on 1070 radial velocity measurements of starsdistributed in 39 fields measuring 4 deg x 4 deg. The PPO series ofFehrenbach et al. (1987) and Duflot et al. (1990) is continued using theFehrenbach objective prism method.
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Besorolás csoportokba:
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Pozíciós és asztrometriai adatok
| Csillagkép: | Kis Kutya |
| Rektaszcenzió: | 07h10m49.86s |
| Deklináció: | +09°22'40.4" |
| Vizuális fényesség: | 7.641 |
| Távolság: | 166.945 parszek |
| RA sajátmozgás: | -3.6 |
| Dec sajátmozgás: | -0.4 |
| B-T magnitude: | 7.632 |
| V-T magnitude: | 7.641 |
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