Arthur Nelson Cox
Affiliations: | 1955- | Los Alamos National Laboratory, Los Alamos, NM, United States |
Area:
theoretical astrophysicsWebsite:
https://baas.aas.org/pub/arthur-nelson-cox-1927-2013Google:
"Arthur Nelson Cox"Bio:
(1927 - 2013)
http://www.legacy.com/obituaries/lamonitor/obituary.aspx?pid=163780429
http://adsabs.harvard.edu/abs/1953PhDT.........1C
http://articles.adsabs.harvard.edu//full/1954ApJ...119..188C/0000196.000.html
Parents
Sign in to add mentorJames Cuffey | grad student | 1953 | Indiana University Bloomington | |
Frank Kelley Edmondson | grad student | 1953 | Indiana University Bloomington | |
John Henry Barrows Irwin | grad student | 1953 | Indiana University Bloomington | |
(A Study of the Galactic Cluster NGC 2287.) |
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Publications
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Guzik JA, Watson LS, Cox AN. (2005) Can enhanced diffusion improve helioseismic agreement for solar models with revised abundances? Astrophysical Journal. 627: 1049-1056 |
Cox AN, Guzik JA. (2004) Theoretical prediction of an observed solar g-mode Astrophysical Journal. 613 |
Cox AN. (2003) A Pulsation Mechanism for GW Virginis Variables The Astrophysical Journal. 585: 975-982 |
Guzik JA, Kaye AB, Bradley PA, et al. (2000) Driving the gravity-mode pulsations in y doradus variables Astrophysical Journal. 542 |
Cox AN, Pilachowski CA. (2000) Allen's astrophysical quantities Physics Today. 53: 77-78 |
Cox AN. (1998) Theoretical Period Changes in Yellow Giant Pulsators The Astrophysical Journal. 496: 246-252 |
Templeton MR, McNamara BJ, Guzik JA, et al. (1997) A new pulsation spectrum and asteroseismology of {delta} Scuti The Astronomical Journal. 114: 1592 |
Christensen-Dalsgaard J, Dappen W, Ajukov SV, et al. (1996) The Current State of Solar Modeling Science (New York, N.Y.). 272: 1286-92 |
Guzik JA, Cox AN. (1995) Early solar mass loss, element diffusion, and solar oscillation frequencies Astrophysical Journal. 448: 905-914 |
Guzik JA, Cox AN. (1993) Using solar p-modes to determine the convection zone depth and constrain diffusion-produced composition gradients Astrophysical Journal. 411: 394-401 |