Carbon isotope and magneto stratigraphy of the Cretaceous (Barremian-Aptian) Pabellon Formation, Chanarcillo Basin, Chile

Gregory D. Price; Ben Dashwood; Graeme K. Taylor; Robert M. Kalin; Neil Ogle

doi:10.1016/j.cretres.2007.04.008

Carbon isotope and magneto stratigraphy of the Cretaceous (Barremian-Aptian) Pabellon Formation, Chanarcillo Basin, Chile

Gregory D. Price^*, Ben Dashwood, Graeme K. Taylor, Robert M. Kalin, Neil Ogle

^*Corresponding author for this work

School of Geography, Earth and Environmental Sciences

Queen's University Belfast

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	183-191
Number of pages	0
Journal	Cretaceous Research
Volume	29
Issue number	2
DOIs	https://doi.org/10.1016/j.cretres.2007.04.008
Publication status	Published - 2008

Keywords

carbon isotope
chile
Chanarcillo Basin
Aptian

Access to Document

10.1016/j.cretres.2007.04.008

Cite this

@article{7c6a0c8129904da3b3999f3b902d0af3,

title = "Carbon isotope and magneto stratigraphy of the Cretaceous (Barremian-Aptian) Pabellon Formation, Chanarcillo Basin, Chile",

keywords = "carbon isotope, chile, Chanarcillo Basin, Aptian",

author = "Price, \{Gregory D.\} and Ben Dashwood and Taylor, \{Graeme K.\} and Kalin, \{Robert M.\} and Neil Ogle",

year = "2008",

doi = "10.1016/j.cretres.2007.04.008",

language = "English",

volume = "29",

pages = "183--191",

journal = "Cretaceous Research",

issn = "0195-6671",

publisher = "Academic Press",

number = "2",

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TY - JOUR

T1 - Carbon isotope and magneto stratigraphy of the Cretaceous (Barremian-Aptian) Pabellon Formation, Chanarcillo Basin, Chile

AU - Price, Gregory D.

AU - Dashwood, Ben

AU - Taylor, Graeme K.

AU - Kalin, Robert M.

AU - Ogle, Neil

PY - 2008

Y1 - 2008

KW - carbon isotope

KW - chile

KW - Chanarcillo Basin

KW - Aptian

U2 - 10.1016/j.cretres.2007.04.008

DO - 10.1016/j.cretres.2007.04.008

M3 - Article

SN - 0195-6671

VL - 29

SP - 183

EP - 191

JO - Cretaceous Research

JF - Cretaceous Research

IS - 2

ER -