[1]
|
B. E. J. Pagel, “Nucleosynthesis and the Chemical Evolution of Galaxies,” Cambridge University Press, Cambridge, 1997.
|
[2]
|
F. Matteucci, “The Chemical Evolution of the Galaxy,” Kluwer Academic Publishers, Dordrecht, 2003.
doi:10.1007/978-94-010-0967-6
|
[3]
|
F. X. Timmes, S. E. Woosley and T. A. Weaver, “Galactic Chemical Evolution: Hydrogen through Zinc,” The Astrophysical Journal Supplement, Vol. 98, No. 2, 1995, pp. 617-658. doi:10.1086/192172
|
[4]
|
C. Chiappini, F. Matteucci and R. Gratton, “The Chemical Evolution of the Galaxy: The Two-Infall Model,” The Astrophysical Journal, Vol. 477, No. 2, 1997, pp. 765-780. doi:10.1086/303726
|
[5]
|
A. Alibés, J. Labay and R. Canal, “Galactic Chemical Abundance Evolution in the Solar Neighborhood up to the Iron Peak,” Astronomy and Astrophysics, Vol. 370, No. 3, 2001, pp. 1103-1121.
doi:10.1051/0004-6361:20010296
|
[6]
|
F. Matteucci, E. Spitoni, S. Recchi and R. Valiante, “The Effect of Different Type Ia Supernova Progenitors on Galactic Chemical Evolution,” Astronomy and Astrophysics, Vol. 501, No. 2, 2009, pp. 531-538.
doi:10.1051/0004-6361/200911869
|
[7]
|
C. Kobayashi and K. Nomoto, “The Role of Type Ia Supernovae in Chemical Evolution. I. Lifetime of Type Ia Supernovae and Metallicity Effect,” The Astrophysical Journal, Vol. 707, No. 2, 2009, pp. 1466-1484.
doi:10.1088/0004-637X/707/2/1466
|
[8]
|
C. Kobayashi and N. Nakasato, “Chemodynamical Simulations of the Milky Way Galaxy,” The Astrophysical Journal, Vol. 729, No. 1, 2011, pp. 16-32.
doi:10.1088/0004-637X/729/1/16
|
[9]
|
S. Sahijpal and G. Gupta, “Numerical Simulation of the Galactic Chemical Evolution: The Revised Solar Abundance,” Meteoritics and Planetary Science Journal, Vol. 48, No. 6, 2013, pp. 1007-1033. doi:10.1111/maps.12123
|
[10]
|
M. Asplund, N. Grevesse, A. J. Sauval and P. Scott, “The Chemical Composition of the Sun,” Annual Review of Astronomy and Astrophysics, Vol. 47, No. 1, 2009, pp. 481-522. doi:10.1146/ annurev.astro.46.060407.145222
|
[11]
|
E. Anders and N. Grevesse, “Abundances of the Elements —Meteoritic and Solar,” Geochimica et Cosmochimica Acta, Vol. 53, No. 1, 1989, pp. 197-214.
doi:10.1016/0016-7037(89)90286-X
|
[12]
|
B. Edvardsson, J. Andersen, B. Gustafsson, D. L. Lambert, P. E. Nissen and J. Tomkin, “The Chemical Evolution of the Galactic Disk—Part One—Analysis and Results,” The Astrophysical Journal, Vol. 275, No. 1, 1993, pp. 101-152.
|
[13]
|
H. Meusinger, B. Stecklum and H. G. Reimann, “The AgeMetallicity-Velocity Dispersion Relation in the Solar Neighborhood and a Simple Evolution Model,” Astronomy and Astrophysics, Vol. 245, No. 1, 1991, pp. 57-74.
|
[14]
|
H. J. Rocha-Pinto, W. J. Maciel, J. Scalo and C. Flynn, “Chemical Enrichment and Star Formation in the Milky Way Disk. I. Sample Description and Chromospheric AgeMetallicity Relation,” Astronomy and Astrophysics, Vol. 358, No. 3, 2000, pp. 850-868.
|
[15]
|
S. Sahijpal, “Galactic Chemical Evolution: The Star Formation Rate in the Early Galaxy,” 39th COSPAR Scientific Assembly, Mysore, 14-22 July 2012, p.1651.
|
[16]
|
M. A. Dopita and S. D. Ryder, “On the Law of Star Formation in Disk Galaxies,” The Astrophysical Journal, Vol. 430, No. 1, 1994, pp. 163-178. doi:10.1086/174390
|
[17]
|
A. I. Karakas and J. C. Lattanzio, “Stellar Models and Yields of Asymptotic Giant Branch Stars,” Publications of the Astronomical Society of Australia, Vol. 24, No. 3, 2007, pp. 103-117. doi:10.1071/AS07021
|
[18]
|
S. E. Woosley and T. A. Weaver, “The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis,” The Astrophysical Journal Supplement, Vol. 101, 1995, pp. 181-235.
doi:10.1086/192237
|
[19]
|
K. Iwamoto, F. Brachwitz, K. Nomoto, N. Kishimoto, H. Umeda, W. R. Hix and F. K. Thielemann, “Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation,” The Astrophysical Journal Supplement, Vol. 125, No. 2, 1999, pp. 439-462.
doi:10.1086/313278
|
[20]
|
G. A. Tammann, W. Loefler and A. Schroder, “The Galactic Supernova Rate,” The Astrophysical Journal Supplement, Vol. 92, No. 2, 1994, pp. 487-493.
doi:10.1086/192002
|