Cooling rates of type I chondrules from Renazzo: Implications for chondrule formation-Reference-Cited by-同舟云学术

Cooling rates of type I chondrules from Renazzo: Implications for chondrule formation

Published:2018-01-15 Issue:5 Volume:53 Page:984-1005
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Chaumard Noël¹²^ORCID,Humayun Munir³,Zanda Brigitte¹,Hewins Roger H.¹⁴

Affiliation:

1. Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie; Sorbonne Universités; Muséum national d'histoire naturelle; UPMC Université Paris 06; UMR CNRS 7590; IRD; UMR 206; CP 52, 57 rue Cuvier 75231 Paris Cedex 05 France

2. Department of Geoscience; WiscSIMS; University of Wisconsin-Madison; 1215 W. Dayton Street Madison Wisconsin 53706-1632 USA

3. Department of Earth, Ocean & Atmospheric Science, and National High Magnetic Field Laboratory; Florida State University; Tallahassee Florida 32310 USA

4. Department of Earth & Planetary Sciences; Rutgers University; Piscataway New Jersey 08855 USA

Funder

Agence Nationale de la Recherche

National Aeronautics and Space Administration

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1111/maps.13040/fullpdf

Reference87 articles.

1. Questions, questions: Can the contradictions between the petrologic, isotopic, thermodynamic, and astrophysical constraints on chondrule formation be resolved?;Alexander;Meteoritics & Planetary Science,2012