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Conference Paper

Pb-U-Th isotopic evolution of the D’Orbigny angrite

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons101028

Jagoutz,  E.
Cosmochemistry, Max Planck Institute for Chemistry, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons101038

Jotter,  R.
Cosmochemistry, Max Planck Institute for Chemistry, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons101330

Varela,  M. E.
Cosmochemistry, Max Planck Institute for Chemistry, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons101388

Zartman,  R.
Cosmochemistry, Max Planck Institute for Chemistry, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons101110

Lugmair,  G. W.
Cosmochemistry, Max Planck Institute for Chemistry, Max Planck Society;

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Citation

Jagoutz, E., Jotter, R., Varela, M. E., Zartman, R., Kurat, G., & Lugmair, G. W. (2002). Pb-U-Th isotopic evolution of the D’Orbigny angrite. In Lunar and Planetary Science XXXIII. Houston/TX: Lunar and Planetary Institute.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-9174-9
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