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Statistical analysis of Fe abundances gradients in the Galaxy

     

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[1]Shaver, P. A., McGee, R. X., Newton, L. M. et al., The galactic abundance gradient, MNRAS, 983, 204: 53.[2]Amnuel, P. R., The features of chemical abundances in Galactic planetary nebulae, MNRAS, 993, 26: 263.[3]Maciel, W. J., Kǒppen, J., Abundance gradents from disk planetary nebulae: O, Ne, S and Ar, A&A, 994, 282, 436.[4]Maciel, W. J., Abundance gradients from planetary nebulae in the galactic disk, IAU Samp., 997, 80: 397.[5]Maciel, W. J., Quireza, C., Abundance gradients in the outer galactic disk from planetary nebulae, A&A, 999, 345: 629.[6]Lennon, D. J., Dufton, P. L., Fitzsimmons, A. et al., Dolidze 25: a metal-deficient galactic open cluster, A&A, 990, 240: 349.[7]Fitzsimmons, A., Dufton, P. L., Rolleston, W. R. J., A comparison of oxygen and nitrogen abundances in young clusters and associations and in the interstellar gas, MNRAS, 992, 259: 489.[8]Kilian, J., Montenbruck, O., Nissen, P. E., The galactic distribution of chemical elements as derived from B-stars in open clusters, A&A, 994, 284: 437.[9]Kaufer, A., Szeifert, T., Krenzin, R. et al., The galactic abundance gradients traced by B-type stars, A&A, 994, 289: 740.[10]Smartt, S. J., Dufton, P. L., Rolleston, W. R. J., A metal deficient early B-type star near the edge of the galactic disk, A&A, 996, 305: 64.[11]Smartt, S. J., Dufton, P. L., Rolleston, W. R. J., The chemical composition towards the galactic anti-centre, A&A, 996, 30: 23.[12]Binette, L., Dopita, M. A., D'Odorico, S. et al., The galactic abundance gradient from supernova remnant observations, A&A, 982, 5: 35.[13]Dauphole, B., Geffert, M., Colin, J. et al., The kinematics of globular clusters, apocentric distances and a halo metallicity gradient, A&A, 996, 33: 9.[14]Marsakov, V. A., Shevelev, Y. G., Catalogue of ages, metallicities, orbital elements and other parameters for nearby F stars, BICDS, 995, 47: 3.[15]Cayrel de Strobel, G., Soubiran, C., Friel, E. D. et al., A catalogue of [Fe/H] determinations: 996 edition, A&AS, 997, 24: 299.[16]Barbier-Brossat, M., Petit, M., Catalogue bibliographique de vitesses radials stellaires, A&AS, 990, 85: 885.[17]Andersen, J., Nordstrǒm, B., Radial velocities of bright southern stars. V. 46 population Ⅱ F stars and related stars, A&AS, 985, 62: 355.[18]Nordstrǒm, B., Anderson, J., Radal velocities of bright southern stars. IV. 55A-and F-type HR and FK stars, A&AS, 985, 6: 53.[19]Perryman, M. A. C., Lindegren, L., Kovalevsky, J. et al., The Hipparcos Catalog, A&A, 997, 323: L49.[20]Allen, C., Santillán, A., An improved model of the galactic mass distribution for orbit computations, RMAA, 99, 22: 255.[21]Allen, C., Martos, M. A., A simple realistic model of the galactic mass distribution for orbit computations, RMAA, 986, 3: 37.[22]Press, W. H., Teukolsky, S. A., Vetterling, W. T., Numrical Recipes in C, The Art of Scientific Computing, 2nd ed., Cambridge: Cambridge University Press, 993.[23]Johnson, D. R. H., Soderblom, D. R., Calculating galactic space velocities and their uncertainties, with an application to the Ursa Major group, AJ, 987, 93: 864.

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