The evolution of the Galactic metallicity gradient from high-resolution spectroscopy of open clusters
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Laura Magrini | Paola Sestito | Daniele Galli | Sofia Randich | S. Randich | L. Magrini | D. Galli | P. Sestito
[1] J. Bernard-Salas,et al. Planetary nebulae abundances and stellar evolution , 2006, astro-ph/0608001.
[2] D. O. Astronomy,et al. Open clusters as key tracers of Galactic chemical evolution. III. Element abundances in Berkeley 20 , 2008, 0807.2313.
[3] L. Pasquini,et al. Abundances of four open clusters from solar stars , 2008, 0806.2280.
[4] E. Friel,et al. ABUNDANCES OF RED GIANTS IN OLD OPEN CLUSTERS. III. NGC 7142 , 2008 .
[5] S. Villanova,et al. Old open clusters as key tracers of Galactic chemical evolution II. Iron and elemental abundances in NGC 2324, NGC 2477, NGC 2660, NGC 3960, and Berkeley 32 , 2008 .
[6] C. M. Bidin,et al. The old open cluster NGC 2112: updated estimates of fundamental parameters based on a membership analysis , 2008, 0802.3243.
[7] F. Palla,et al. Detection of the lithium depletion boundary in the young open cluster IC 4665 , 2007, 0712.0226.
[8] P. Frinchaboy,et al. Old open clusters in the outer Galactic disk , 2007, 0709.2126.
[9] E. Corbelli,et al. The building up of the disk galaxy M 33 and the evolution of the metallicity gradient , 2007, 0704.3187.
[10] Santiago,et al. Detailed chemical composition of Galactic Cepheids. A determination of the Galactic abundance gradie , 2007, astro-ph/0701499.
[11] C. Quireza,et al. Time variation of radial gradients in the Galactic disk: electron temperatures and abundances , 2007, astro-ph/0701337.
[12] S. Randich,et al. Element abundances in the metal-rich open cluster NGC 6253 , 2007, astro-ph/0701182.
[13] P. François,et al. Abundance gradients in the Milky Way for α elements, iron peak elements, barium, lanthanum, and europium , 2006, astro-ph/0609813.
[14] U. Washington,et al. The absolute motion of the peculiar cluster NGC 6791 , 2006, astro-ph/0610546.
[15] L. Morbidelli,et al. The chemical gradient of oxygen in the Galaxy from planetary nebulae , 2006 .
[16] J. Bernard-Salas,et al. Planetary nebulae abundances and stellar evolution II , 2006, 1005.3042.
[17] K. Cunha,et al. Planetary Nebula Abundances and Morphology: Probing the Chemical Evolution of the Milky Way , 2006, astro-ph/0607480.
[18] S. Randich,et al. Old open clusters as key tracers of Galactic chemical evolution. I. Fe abundances in NGC 2660, NGC 3 , 2006, astro-ph/0607438.
[19] M. R. Haas,et al. Abundance Gradients in the Galaxy , 2006 .
[20] L. Pasquini,et al. Element abundances of unevolved stars in the open cluster M 67 , 2006, astro-ph/0601239.
[21] Giampaolo Piotto,et al. NGC 6791: An Exotic Open Cluster or the Nucleus of a Tidally Disrupted Galaxy? , 2005, astro-ph/0512650.
[22] J. Ostriker,et al. A simple model for the evolution of disc galaxies: the Milky Way , 2005, astro-ph/0505594.
[23] A. Helmi,et al. Chemical Abundances and Mixing in Stars in the Milky Way and Its Satellites , 2006 .
[24] L. Pasquini,et al. Chemical abundances and mixing in stars in the milky way and its satellites : proceedings of the ESO-Arcetri Workshop held in Castiglione della Pescaia, Italy, 13-17 September, 2004 , 2006 .
[25] Bangalore,et al. Elemental abundance survey of the Galactic thick disc , 2005, astro-ph/0512505.
[26] A. Bragaglia,et al. The Bologna Open Cluster Chemical Evolution Project: Midterm Results from the Photometric Sample , 2005, astro-ph/0511020.
[27] R. Jeffries,et al. Elemental abundances in the Blanco 1 open cluster , 2005, astro-ph/0508606.
[28] Astrophysics,et al. Spectroscopic Abundance Analysis of Dwarfs in the Young Open Cluster IC 4665 , 2005, astro-ph/0508387.
[29] E. Friel,et al. Abundances of Red Giants in Old Open Clusters. II. Berkeley 17 , 2005 .
[30] G. Carraro,et al. Metal Abundances in Extremely Distant Galactic Old Open Clusters. II. Berkeley 22 and Berkeley 66 , 2005, astro-ph/0504282.
[31] B. Carney,et al. Elemental Abundance Ratios in Stars of the Outer Galactic Disk. I. Open Clusters , 2005, astro-ph/0504193.
[32] M. Mollá,et al. A grid of chemical evolution models as a tool to interpret spiral and irregular galaxies data , 2005 .
[33] B. Edvardsson,et al. Chemical composition of evolved stars in the open cluster NGC 7789 , 2005 .
[34] M. Mollá,et al. Low and intermediate mass star yields: The evolution of carbon abundances , 2004, astro-ph/0411746.
[35] F. Mannucci,et al. The Supernova rate per unit mass , 2004, astro-ph/0411450.
[36] C. Chiappini,et al. Interpretation of Abundance Ratios , 2004, Publications of the Astronomical Society of Australia.
[37] G. Carraro,et al. Metal Abundances in Extremely Distant Galactic Old Open Clusters. I. Berkeley 29 and Saurer 1 , 2004, astro-ph/0406679.
[38] L. Pasquini,et al. Detailed chemical composition of the open cluster IC 4651: The iron peak, α elements, and Li , 2004, astro-ph/0406113.
[39] R. Gratton,et al. Iron abundances from high-resolution spectroscopy of the open clusters NGC 2506, NGC 6134, and IC 4651 , 2004, astro-ph/0404298.
[40] Explosive Yields of Massive Stars from Z = 0 to Z = Z? , 2004, astro-ph/0402625.
[41] K. S. Boer. The contribution of halo red giant mass loss to the high-velocity gas falling onto the Milky Way disk , 2004, astro-ph/0402630.
[42] -INAF,et al. The evolution of the Milky Way from its earliest phases: Constraints on stellar nucleosynthesis , 2004, astro-ph/0401499.
[43] Garching,et al. The age of the oldest Open Clusters , 2003, astro-ph/0310363.
[44] J. Lépine,et al. The Galactic abundance gradient from Cepheids - V. Transition zone between 10 and 11 kpc , 2004 .
[45] E. Friel,et al. Abundances of Red Giants in the Old Open Cluster Collinder 261 , 2003 .
[46] W. Cochran,et al. Searching for Planets in the Hyades. IV. Differential Abundance Analysis of Hyades Dwarfs , 2003 .
[47] S. Randich,et al. The evolution of lithium depletion in young open clusters: NGC 6475 , 2003, astro-ph/0305394.
[48] G. Chabrier. Galactic Stellar and Substellar Initial Mass Function , 2003, astro-ph/0304382.
[49] W. Gieren,et al. The galactic abundance gradient from Cepheids - IV. New results for the outer disc , 2003 .
[50] J. Hou,et al. On the Galactic Disk Metallicity Distribution from Open Clusters. I. New Catalogs and Abundance Gradient , 2002, astro-ph/0212542.
[51] W. J. Maciel,et al. An estimate of the time variation of the O/H radial gradient from planetary nebulae , 2002, astro-ph/0210470.
[52] Nathan D. Miller,et al. Metallicities of Old Open Clusters , 2002 .
[53] D. Soderblom,et al. Spectroscopic Abundances of Solar-Type Dwarfs in the Open Cluster M34 (NGC 1039) , 2001 .
[54] S. Corder,et al. Field Stars, Open Clusters, and the Galactic Abundance Gradient , 2001, astro-ph/0106136.
[55] C. Chiappini,et al. Abundance Gradients and the Formation of the Milky Way , 2001, astro-ph/0102134.
[56] G. González,et al. Elemental Abundances in the Inner Galaxy Open Cluster M11 , 2000 .
[57] L. Deharveng,et al. Oxygen and helium abundances in Galactic H ii regions — II. Abundance gradients , 2000 .
[58] Koichi Iwamoto,et al. Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation , 1999 .
[59] G. Worthey,et al. Publications of the Astronomical Society of the Pacific The Distribution Of Heavy Elements In Spiral And Elliptical Galaxies , 1999 .
[60] France.,et al. Chemo-spectrophotometric evolution of spiral galaxies — I. The model and the Milky Way , 1999, astro-ph/9902148.
[61] G. Carraro,et al. On the Galactic disc age–metallicity relation , 1997, astro-ph/9707185.
[62] K. Ashman,et al. Some Revised Observational Constraints on the Formation and Evolution of the Galactic Disk , 1997, astro-ph/9709122.
[63] F. Ferrini,et al. Evolution of Spiral Galaxies. VII. Time Evolution of the Radial Distributions of Abundances , 1997 .
[64] C. Chiappini,et al. The Chemical Evolution of the Galaxy: The Two-Infall Model , 1996, astro-ph/9609199.
[65] P. Sackett. Does the Milky Way Have a Maximal Disk? , 1996, astro-ph/9608164.
[66] F. Ferrini,et al. Evolution of Spiral Galaxies. VI. Radial Distributions of Abundances in External Galaxies , 1996 .
[67] The Old Open Cluster, Berkeley 66 , 1996 .
[68] M. Tosi. Comparison of Chemical Evolution Models for the Galactic Disk , 1995, astro-ph/9512096.
[69] E. D. Friel,et al. The Old Open Clusters of the Milky Way , 1995 .
[70] F. Ferrini,et al. Evolution of spiral galaxies. III. Application of the multiphase model to the galactic disk , 1994 .
[71] Randy L. Phelps,et al. Development of the Galactic Disk: A Search for the Oldest Open Cluster , 1994 .
[72] S. Holt,et al. Back to the Galaxy , 1993 .
[73] G. Gilmore,et al. The distribution of low-mass stars in the Galactic disc , 1993 .
[74] F. Ferrini,et al. Evolution of spiral galaxies. I - Halo-disk connection for the evolution of the solar neighborhood , 1992 .
[75] E. Friel,et al. Chemical composition of open clusters. I. Fe/H from high-resolution spectroscopy. II. C/H and C/Fe in F dwarfs from high-resolution spectroscopy , 1990 .
[76] S. M. Fall,et al. Chemical evolution of the galactic disk with radial gas flows. , 1985 .
[77] J. Audouze. Nucleosynthesis and Chemical Evolution of Galaxies , 1983 .
[78] K. Janes. Evidence for an abundance gradient in the galactic disk , 1979 .
[79] W. Arnett,et al. Evolution Of Galaxies .2. Chemical Evolution Coefficients , 1973 .
[80] W. Arnett,et al. The Evolution of Galaxies. II. Chemical Evolution Coefficients , 1973 .
[81] E. Salpeter. The Luminosity function and stellar evolution , 1955 .