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, University of Notre Dame
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Results 1 - 5 of 5
The case of the disappearing CN-strong AGB stars in Galactic globular clusters -- Preliminary Results
Volume 5, Issue 16 - article #9
S. W. Campbell
(1 and 2),
D. Yong
(3),
E. C. Wylie-de Boer
(3),
R. J. Stancliffe
(2),
J. C. Lattanzio
(2),
G. C. Angelou
(2),
F. Grundahl
(4),
C. Sneden
(5)
((1) Departament de Fisica i Enginyeria Nuclear, Universitat Politecnica de Catalunya, Barcelona, Spain,
(2) Centre for Stellar and Planetary Astrophysics, Monash University, Australia,
(3) Research School of Astronomy and Astrophysics, Australian National University, Australia,
(4) Department of Physics and Astronomy, Aarhus University, Denmark,
(5) Department of Astronomy and McDonald Observatory, University of Texas, Austin, USA)
arXiv.org - Astrophysics - Volume: 2010, Issue: 16 Apr
arXiv:1004.2249
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Element enhancements along the entire AGB phase
Volume 3, Issue 43 - article #4
E. C. Wylie-de Boer
,
P. L. Cottrell
arXiv.org - Astrophysics - Volume: 2008, Issue: 23 Oct
arXiv:0810.3056
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s
- and
r
-Process Element Abundances in the CMD of 47 Tucanæ Using the Robert Stobie Spectrograph on SALT
Volume 3, Issue 26 - article #15
C. C. Worley
,
P. L. Cottrell
and
E. C. Wylie de Boer
Publications of the Astronomical Society of Australia - Volume: 25, Issue: 2
Abstract
|
Full Text
|
PDF (736 KB)
Heavy-Element Abundances in Giant Stars in 47 Tucanae
Volume 1, Issue 34 - article #2
E. C. Wylie
,
P. L. Cottrell
,
C. A. Sneden
,
and
J. C. Lattanzio
The Astrophysical Journal - Volume649, Issue 1
ABSTRACT
,
FULL TEXT
,
PDF
(420 kB),
PS
Heavy Element Abundances in Giant Stars of 47 Tuc
Volume 1, Issue 18 - article #9
E. C. Wylie
,
P. L. Cottrell
,
C. A. Sneden
,
J. C. Lattanzio
astro-ph/0605538 [
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Results 1 - 5 of 5
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