From: The chemical evolution of the Milky Way: the Three Infall Model
Mon Not R Astron Soc. 2013;436(2):1648-1658. doi:10.1093/mnras/stt1681
Mon Not R Astron Soc | © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
From: The chemical evolution of the Milky Way: the Three Infall Model
Mon Not R Astron Soc. 2013;436(2):1648-1658. doi:10.1093/mnras/stt1681
Mon Not R Astron Soc | © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
From: The chemical evolution of the Milky Way: the Three Infall Model
Mon Not R Astron Soc. 2013;436(2):1648-1658. doi:10.1093/mnras/stt1681
Mon Not R Astron Soc | © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
From: The chemical evolution of the Milky Way: the Three Infall Model
Mon Not R Astron Soc. 2013;436(2):1648-1658. doi:10.1093/mnras/stt1681
Mon Not R Astron Soc | © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
From: The chemical evolution of the Milky Way: the Three Infall Model
Mon Not R Astron Soc. 2013;436(2):1648-1658. doi:10.1093/mnras/stt1681
Mon Not R Astron Soc | © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
From: The chemical evolution of the Milky Way: the Three Infall Model
Mon Not R Astron Soc. 2013;436(2):1648-1658. doi:10.1093/mnras/stt1681
Mon Not R Astron Soc | © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
From: The chemical evolution of the Milky Way: the Three Infall Model
Mon Not R Astron Soc. 2013;436(2):1648-1658. doi:10.1093/mnras/stt1681
Mon Not R Astron Soc | © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society