Chemodynamicsl model of the Galaxy: abundance gradients predicted for H II regions and planetary nebulae.

Details Chemodynamicsl model of the Galaxy: abundance gradients predicted for H II regions and planetary nebulae. Chemodynamicsl model of the Galaxy: abundance gradients predicted for H II regions and planetary nebulae.

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998rmxac...7..216a&link_type=toc

Revista Mexicana de Astronomia y Astrofisica, Ser. Conf., Vol. 7, p. 216

Astronomy and Astrophysics

Astronomy

Galaxy: Chemical Evolution, Galaxy: Dynamical Evolution

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