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Galactic model parameters for field giants separated from field dwarfs by their 2MASS and V apparent magnitudes We present a method which separates field dwarfs and field giants bytheir 2MASS and V apparent magnitudes. This method is based onspectroscopically selected standards and is hence reliable. We appliedit to stars in two fields, SA 54 and SA 82, and we estimated a full setof Galactic model parameters for giants including their total localspace density. Our results are in agreement with the ones given in therecent literature.
| A catalogue of [Fe/H] determinations: 1996 edition A fifth Edition of the Catalogue of [Fe/H] determinations is presentedherewith. It contains 5946 determinations for 3247 stars, including 751stars in 84 associations, clusters or galaxies. The literature iscomplete up to December 1995. The 700 bibliographical referencescorrespond to [Fe/H] determinations obtained from high resolutionspectroscopic observations and detailed analyses, most of them carriedout with the help of model-atmospheres. The Catalogue is made up ofthree formatted files: File 1: field stars, File 2: stars in galacticassociations and clusters, and stars in SMC, LMC, M33, File 3: numberedlist of bibliographical references The three files are only available inelectronic form at the Centre de Donnees Stellaires in Strasbourg, viaanonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5), or viahttp://cdsweb.u-strasbg.fr/Abstract.html
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Observation and Astrometry data
Constellation: | Puppis |
Right ascension: | 06h15m40.46s |
Declination: | -46°07'55.2" |
Apparent magnitude: | 8.276 |
Distance: | 408.163 parsecs |
Proper motion RA: | -3.2 |
Proper motion Dec: | 22.2 |
B-T magnitude: | 8.362 |
V-T magnitude: | 8.284 |
Catalogs and designations:
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