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, University of Notre Dame
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Results 1 - 40 of 40
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
Volume 17, Issue 23 - article #11
Haining Li
,
Wako Aoki
,
Tadafumi Matsuno
,
Qianfan Xing
,
Takuma Suda
,
Nozomu Tominaga
,
Yuqin Chen
,
Satoshi Honda
,
Miho N. Ishigaki
,
Jianrong Shi
The Astrophysical Journal
https://doi.org/10.3847/1538-4357/ac6514
Four-hundred Very Metal-poor Stars studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency. (arXiv:2203.11505v1 [astro-ph.SR])
Volume 17, Issue 12 - article #2
Wako Aoki
,
Haining Li
,
Tadafumi Matsuno
,
Qianfan Xing
,
Yuqin Chen
,
Norbert Christlieb
,
Satoshi Honda
,
Miho N. Ishigaki
,
Jianrong Shi
,
Takuma Suda
,
Nozomu Tominaga
,
Hong-Liang Yan
,
Jingkun Zhao
,
Gang Zhao
http://arxiv.org/abs/2203.11505
Four-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances. (arXiv:2203.11529v1 [astro-ph.SR])
Volume 17, Issue 12 - article #3
Haining Li
,
Wako Aoki
,
Tadafumi Matsuno
,
Qianfan Xing
,
Takuma Suda
,
Nozomu Tominaga
,
Yuqin Chen
,
Satoshi Honda
,
Miho N. Ishigaki
,
Jianrong Shi
,
Jingkun Zhao
,
Gang Zhao
http://arxiv.org/abs/2203.11529
High-precision chemical abundances of Galactic building blocks. The distinct chemical abundance sequence of Sequoia. (arXiv:2111.15423v1 [astro-ph.GA])
Volume 16, Issue 49 - article #4
Tadafumi Matsuno
,
Helmer H. Koppelman
,
Amina Helmi
,
Wako Aoki
,
Miho N. Ishigaki
,
Takuma Suda
,
Zhen Yuan
,
Kohei Hattori
http://arxiv.org/abs/2111.15423
First Star Survivors as Metal-Rich Halo Stars that Experienced Supernova Explosions in Binary Systems. (arXiv:2103.13627v1 [astro-ph.SR])
Volume 16, Issue 13 - article #1
Takuma Suda
,
Takayuki R. Saitoh
,
Yuki Moritani
,
Tadafumi Matsuno
,
Toshikazu Shigeyama
http://arxiv.org/abs/2103.13627
Most Lithium-rich Low-mass Evolved Stars Revealed as Red Clump stars by Asteroseismology and Spectroscopy. (arXiv:2010.02106v1 [astro-ph.SR])
Volume 15, Issue 41 - article #5
Hong-Liang Yan
,
Yu-Tao Zhou
,
Xianfei Zhang
,
Yaguang Li
,
Qi Gao
,
Jian-Rong Shi
,
Gang Zhao
,
Wako Aoki
,
Tadafumi Matsuno
,
Yan Li
,
Xiao-Dong Xu
,
Haining Li
,
Ya-Qian Wu
,
Meng-Qi Jin
,
Benoît Mosser
,
Shao-Lan Bi
,
Jian-Ning Fu
,
Kaike Pan
,
Takuma Suda
,
Yu-Juan Liu
,
Jing-Kun Zhao
,
Xi-Long Liang
http://arxiv.org/abs/2010.02106
s-process enirchment and the origin of barium in ultrafaint dwarf galaxies. (arXiv:2009.10096v1 [astro-ph.GA])
Volume 15, Issue 39 - article #8
Yuta Tarumi
,
Takuma Suda
,
Robert J. J. Grand
,
Freeke van de Voort
,
Shigeki Inoue
,
Naoki Yoshida
http://arxiv.org/abs/2009.10096
Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
Volume 15, Issue 24 - article #12
Tadafumi Matsuno
,
Wako Aoki
,
Luca Casagrande
,
Miho Ishigaki
,
Jianrong Shi
,
Masao Takata
,
Maosheng Xiang
,
David Yong
,
Haining Li
,
Takuma Suda
,
Qianfan Xing
,
Jingkun Zhao
http://arxiv.org/abs/2006.03619
Are Faint Supernovae Responsible for Carbon-enhanced Metal-poor Stars?
Volume 15, Issue 7 - article #15
Yutaka Komiya
,
Takuma Suda
,
Shimako Yamada,
,
Masayuki Y. Fujimoto
The Astrophysical Journal
http://iopscience.iop.org/0004-637X/890/1/66
LAMOST J2217+2104: a new member of carbon-enhanced extremely metal-poor stars with excesses of Mg and Si. (arXiv:1807.11628v1 [astro-ph.SR])
Volume 13, Issue 31 - article #1
Wako Aoki
,
Tadafumi Matsuno
,
Satoshi Honda
,
Miho Ishigaki
,
Haining Li
,
Takuma Suda
,
Yerra Bharat Kummar
http://arxiv.org/abs/1807.11628
Enormous Li Enhancement Preceding Red Giant Phases in Low-mass Stars in the Milky Way Halo
Volume 13, Issue 3 - article #12
Haining Li
,
Wako Aoki
,
Tadafumi Matsuno
,
Yerra Bharat Kumar
,
Jianrong Shi
,
Takuma Suda,
,
Gang Zhao
The Astrophysical Journal Letters
http://iopscience.iop.org/2041-8205/852/2/L31
Enormous Li-enhancement preceding red giant phases in low-mass stars in the Milky Way halo. (arXiv:1801.00090v1 [astro-ph.SR])
Volume 13, Issue 1 - article #3
Haining Li
,
Wako Aoki
,
Tadafumi Matsuno
,
Yerra Bharat Kumar
,
Jianrong Shi
,
Takuma Suda
,
Gang Zhao
http://arxiv.org/abs/1801.00090
Stellar Abundances for Galactic Archaeology IV - Compilation of Stars in Dwarf Spheroidal Galaxies. (arXiv:1703.10009v1 [astro-ph.GA])
Volume 12, Issue 13 - article #2
Takuma Suda
,
Jun Hidaka
,
Wako Aoki
,
Yutaka Katsuta
,
Shimako Yamada
,
Masayuki Y. Fujimoto
,
Yukari Ohtani
,
Miyu Masuyama
,
Kazuhiro Noda
,
Kentaro Wada
http://arxiv.org/abs/1703.10009
Lithium in CEMP-no stars: A new constraint on the lithium depletion mechanism in the early universe. (arXiv:1612.06624v1 [astro-ph.SR])
Volume 11, Issue 52 - article #2
Tadafumi Matsuno
,
Wako Aoki
,
Takuma Suda
,
Haining Li
http://arxiv.org/abs/1612.06624
Population III stars around the Milky Way
Volume 11, Issue 13 - article #7
Yutaka Komiya
,
Takuma Suda
,
Masayuki Y. Fujimoto
arXiv.org - Astrophysics - Volume: 2016, Issue: 25 Mar
arXiv:1603.06096
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The Most Iron-deficient Stars as the Polluted Population III Stars
Volume 10, Issue 29 - article #10
Yutaka Komiya
,
Takuma Suda
,
and
Masayuki Y. Fujimoto
The Astrophysical Journal Letters - Volume: 808, Issue: 2
View article
PDF (595 KB)
The most iron-deficient stars as the polluted population III stars
Volume 10, Issue 25 - article #16
Yutaka Komiya
,
Takuma Suda
,
Masayuki Y. Fujimoto
arXiv.org - Astrophysics - Volume: 2015, Issue: 10 Jul
arXiv:1507.01664
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High-Resolution Spectroscopy of Extremely Metal-Poor Stars from SDSS/SEGUE. II. Binary Fraction
Volume 10, Issue 5 - article #13
Wako Aoki
,
Takuma Suda
,
Timothy C. Beers
,
and
Satoshi Honda
Astronomical Journal - Volume: 149, Issue: 2
View article
PDF (303 KB)
Carbon-enhanced Metal-poor Stars in SDSS/SEGUE. II. Comparison of CEMP-star Frequencies with Binary Population-synthesis Models
Volume 9, Issue 21 - article #63
Young Sun Lee
,
Takuma Suda
,
Timothy C. Beers
,
and
Richard J. Stancliffe
The Astrophysical Journal - Volume: 788, Issue: 2
View article
PDF (410 KB)
The New Model of Chemical Evolution of
r
-process Elements Based on the Hierarchical Galaxy Formation. I. Ba and Eu
Volume 9, Issue 18 - article #11
Yutaka Komiya
,
Shimako Yamada
,
Takuma Suda
,
and
Masayuki Y. Fujimoto
The Astrophysical Journal - Volume: 783, Issue: 2
View article
PDF (2.90 MB)
The New Model of Chemical Evolution of r-process Elements Based on The Hierarchical Galaxy Formation I: Ba and Eu
Volume 9, Issue 5 - article #14
Yutaka Komiya
,
Shimako Yamada
,
Takuma Suda
,
Masayuki Y. Fujimoto
arXiv.org - Astrophysics - Volume: 2014, Issue: 31 Jan
arXiv:1401.6261
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The Stellar Abundances for Galactic Archaeology (SAGA) Database – III. Analysis of enrichment histories for elements and two modes of star formation during the early evolution of the Milky Way
Volume 9, Issue 4 - article #30
Shimako Yamada
,
Takuma Suda
,
Yutaka Komiya
,
Wako Aoki
,
and
Masayuki Y. Fujimoto
Monthly Notices of the Royal Astronomical Society - Volume: 436, Issue: 2
Abstract
Full Text (HTML)
Full Text (PDF)
Current signatures and search for Pop. III stars in the Local Universe
Volume 8, Issue 51 - article #3
Yutaka Komiya
,
Takuma Suda
,
Masayuki Fujimoto
arXiv.org - Astrophysics - Volume: 2013, Issue: 20 Dec
arXiv:1312.5069
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Carbon-enhanced Metal-poor Stars in SDSS/SEGUE. II. Comparison of CEMP Star Frequencies with Binary Population Synthesis Models
Volume 8, Issue 42 - article #3
Young Sun Lee
,
Takuma Suda
,
Timothy C. Beers
,
Sara Lucatello
arXiv.org - Astrophysics - Volume: 2013, Issue: 18 Oct
arXiv:1310.3277
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The Stellar Abundances for Galactic Archaeology (SAGA) Database III - Analysis of Enrichment Histories for Elements and Two Modes of Star Formation during the Early Evolution of Milky Way
Volume 8, Issue 38 - article #12
Shimako Yamada
,
Takuma Suda
,
Yutaka Komiya
,
Wako Aoki
,
Masayuki Y. Fujimoto
arXiv.org - Astrophysics - Volume: 2013, Issue: 20 Sep
arXiv:1309.3430
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Explaining the Sr and Ba Scatter in Extremely Metal-Poor Stars
Volume 8, Issue 9 - article #5
Wako Aoki
,
Takuma Suda
,
Richard Boyd
,
Toshitaka Kajino
,
Michael Famiano
arXiv.org - Astrophysics - Volume: 2013, Issue: 1 Mar
arXiv:1302.6573
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High-Resolution Spectroscopy of Extremely Metal-Poor Stars from SDSS/SEGUE: I. Atmospheric Parameters and Chemical Compositions
Volume 7, Issue 41 - article #4
Wako Aoki
,
Timothy C. Beers
,
Young Sun Lee
,
Satoshi Honda
,
Hiroko Ito
,
Masahide Takada-Hidai
,
Anna Frebel
,
Takuma Suda
,
Masatuki Y. Fujimoto
,
Daniela Carollo
,
Thirupathi Sivarani
arXiv.org - Astrophysics - Volume: 2012, Issue: 12 Oct
arXiv:1210.1946
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]
Stellar Evolution Constraints on the Triple-α Reaction Rate
Volume 6, Issue 44 - article #22
Takuma Suda
,
Raphael Hirschi
and
Masayuki Y. Fujimoto
The Astrophysical Journal - Volume: 741, Issue: 1
Abstract
References
Full text PDF (1.85 MB)
View as HTML
Stellar Evolution Constraints on the Triple-Alpha Reaction Rate
Volume 6, Issue 30 - article #15
Takuma Suda
,
Raphael Hirschi
,
Masayuki Y. Fujimoto
arXiv.org - Astrophysics - Volume: 2011, Issue: 29 Jul
arXiv:1107.4984
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The Stellar Abundances for Galactic Archaeology (SAGA) data base – II. Implications for mixing and nucleosynthesis in extremely metal-poor stars and chemical enrichment of the Galaxy
Volume 6, Issue 11 - article #21
Takuma Suda
,
Shimako Yamada
,
Yutaka Katsuta
,
Yutaka Komiya
,
Chikako Ishizuka
,
Wako Aoki
and
Masayuki Y. Fujimoto
Monthly Notices of the Royal Astronomical Society - Volume: 412, Issue: 2
Abstract
Full Article (HTML)
PDF(4067K)
References
Oxygen and light element synthesis by neutron-capture reactions in metal-free and extremely metal-poor AGB stars
Volume 4, Issue 26 - article #7
Takanori Nishimura
,
Masayuki Aikawa
,
Takuma Suda
,
Masayuki Y. Fujimoto
arXiv.org - Astrophysics - Volume: 2009, Issue: 26 Jun
arXiv:0906.4494
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Hierarchical Formation of the Galactic Halo and the Origin of Hyper Metal-Poor Stars
Volume 4, Issue 16 - article #11
<em >Yutaka Komiya
,
Asao Habe
,
Takuma Suda
,
and
Masayuki Y. Fujimoto</em>
,
The Astrophysical Journal Letters - Volume: 696, Issue: 1
Abstract
|
References
Early-Age Evolution of the Milky Way Related by Extremely Metal-Poor Stars
Volume 4, Issue 13 - article #50
<em >Yutaka Komiya
,
Takuma Suda
,
and
Masayuki Y. Fujimoto</em>
,
The Astrophysical Journal - Volume: 694, Issue: 2
Abstract
|
References
Early-Age Evolution of the Milky Way Related by Extremely Metal-Poor Stars
Volume 4, Issue 2 - article #4
Yutaka Komiya
,
Takuma Suda
,
Masayuki Y. Fujimoto
arXiv.org - Astrophysics - Volume: 2009, Issue: 8 Jan
arXiv:0901.0617
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The IMF of Extremely Metal-Poor Stars and the Probe into the Star-Formation Process of the Milky Way
Volume 2, Issue 43 - article #26
Yutaka Komiya
,
Takuma Suda
,
Asao Habe
,
Masayuki Y. Fujimoto
arXiv.org - Astrophysics - Volume: 2007, Issue: 25 Oct
arXiv:0710.4374
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Evolution of Low-Mass Population III Stars
Volume 2, Issue 39 - article #7
Takuma Suda
,
Masayuki Y. Fujimoto
,
and
Naoki Itoh
The Astrophysical Journal - Volume: 667, Issue: 2
ABSTRACT
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FULL TEXT
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PDF
(502 kB) |
PS
The Origin of Carbon Enhancement and the Initial Mass Function of Extremely Metal-poor Stars in the Galactic Halo
Volume 2, Issue 12 - article #3
Yutaka Komiya
,
Takuma Suda
,
Hiroki Minaguchi
,
Toshikazu Shigeyama
,
Wako Aoki
,
and
Masayuki Y. Fujimoto
The Astrophysical Journal - Volume658, Issue 1
ABSTRACT
,
FULL TEXT WITH ENHANCEMENTS
,
PDF
(622 kB),
PS
The Origin of Carbon Enhancement and the Initial Mass Function of Extremely Metal-poor Stars in the Galactic Halo
Volume 2, Issue 11 - article #4
Yutaka Komiya
,
Takuma Suda
,
Hiroki Minaguchi
,
Toshikazu Shigeyama
,
Wako Aoki
,
and
Masayuki Y. Fujimoto
The Astrophysical Journal - Volume658, Issue 1
ABSTRACT
,
FULL TEXT WITH ENHANCEMENTS
,
PDF
(622 kB),
PS
The Origin of Carbon-Enhancement and Initial Mass Function of Extremely Metal-Poor Stars in the Galactic Halo
Volume 1, Issue 39 - article #10
Yutaka Komiya
,
Takuma Suda
,
Hiroki Minaguchi
,
Toshikazu Shigeyama
,
Wako Aoki
,
Masayuki Y. Fujimoto
ArXiv - Astrophysics
astro-ph/0610670 [
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Various Modes of Helium Mixing in Globular Cluster Giants and Their Possible Effects on the Horizontal Branch Morphology
Volume 1, Issue 3 - article #21
Takuma Suda
,
Masayuki Y. Fujimoto
(Hokkaido University)
ArXiv - Astrophysics
astro-ph/0602189 [
abs
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other
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Results 1 - 40 of 40
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