Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-30T21:19:28.906Z Has data issue: false hasContentIssue false
  • English
  • Français

A Comparison of Chemical Evolution between the Milky Way and M31 Galaxy

Published online by Cambridge University Press:  01 August 2006

J. Yin ,
J.L. Hou ,
R.X. Chang ,
S. Boissier  and
N. Prantzos
J. Yin
Affiliation:
Shanghai Astronomical Observatory, CAS, Shanghai, 200030, China email: [email protected], [email protected], [email protected]
J.L. Hou
Affiliation:
Shanghai Astronomical Observatory, CAS, Shanghai, 200030, China email: [email protected], [email protected], [email protected]
R.X. Chang
Affiliation:
Shanghai Astronomical Observatory, CAS, Shanghai, 200030, China email: [email protected], [email protected], [email protected]
S. Boissier
Affiliation:
Laboratoire d'Astrophysique de Marseillee, Traverse du Syphon-Les trois lucs BP8, 13376 Marseille cedex 12, France email: [email protected]
N. Prantzos
Affiliation:
Institut d'Astrophysique de Paris, CNRS, 98bis Bd Arage, 75014, Paris, France email: [email protected]
Rights & Permissions [Opens in a new window]

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Andromeda galaxy (M31,NGC224) is the biggest spiral in the Local Group. By studying the star formation history(SFH) and chemical evolution of M31, and comparing with the Milky Way Galaxy, we are able to understand more about the formation and evolution of spiral galaxies.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 313
Copyright
Copyright © International Astronomical Union 2007