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Metallicities and activities of southern stars Aims. We present the results from high-resolution spectroscopicmeasurements to determine metallicities and activities of bright starsin the southern hemisphere.  Methods: We measured the iron abundances([Fe/H]'s) and chromospheric emission indices (log h{R}'{HK})of 353 solar-type stars with V = 7.5-9.5. [Fe/H] abundances aredetermined using a custom χ2 fitting procedure within alarge grid of Kurucz model atmospheres. The chromospheric activitieswere determined by measuring the amount of emission in the cores of thestrong Caii HK lines.  Results: Our comparison of the metallicity sampleto other [Fe/H] determinations was found to agree at the ±0.05dex level for spectroscopic values and at the ±0.1 dex level forphotometric values. The distribution of chromospheric activities isdescribed by a bimodal distribution, agreeing with the conclusions fromother works. Also an analysis of Maunder minimum status was attempted,and it was found that 6 ± 4 stars in the sample could be in aMaunder minimum phase of their evolution and hence the Sun should onlyspend a few per cent of its main sequence lifetime in Maunder minimum.Based on observations made with the ESO telescopes at the La SillaParanal observatory under programme ID's 076.C-0578(B) and077.C-0192(A). Table 4 is only available in electronic form at the CDSvia anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/485/571
 
  |  UBV photometry of HD stars in the fields of selected cataclysmic variables. Not Available
 
  |  Dwarf K and M stars in the southern hemisphere. Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1972AJ.....77..486U&db_key=AST
 
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Datos observacionales y astrométricos
| Constelación: | Virgo |  
    | Ascensión Recta: | 13h44m12.92s |  
    | Declinación: | -08°29'17.9" |  
    | Magnitud Aparente: | 9.139 |  
    
        | Distancia: | 40.323 parsecs |  
        
    
    | Movimiento Propio en Ascensión Recta: | -8.2 |  
    | Movimiento Propio en Declinación: | -8.4 |  
    | B-T magnitude: | 10.208 |  
    | V-T magnitude: | 9.228 |  
    
 
 
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