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H. Sameshima
H. Sameshima
University of Tokyo
Astronomy
Astrophysics
Physics
Stars
Galaxy
5
Papers
7
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0
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Possible Progression of Mass-flow Processes around Young Intermediate-mass Stars Based on High-resolution Near-infrared Spectroscopy. I. Taurus
2019
The Astrophysical Journal
Chikako Yasui
Satoshi Hamano
Kei Fukue
Sohei Kondo
H. Sameshima
Keiichi Takenaka
Noriyuki Matsunaga
Yuji Ikeda
Hideyo Kawakita
Shogo Otsubo
Ayaka Watase
Daisuke Taniguchi
Misaki Mizumoto
Natsuko Izumi
Naoto Kobayashi
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Citations (4)
Possible progression of mass flow processes around young intermediate-mass stars based on high-resolution near-infrared spectroscopy. I. Taurus.
2019
arXiv: Solar and Stellar Astrophysics
Chikako Yasui
Satoshi Hamano
Kei Fukue
Sohei Kondo
H. Sameshima
Keiichi Takenaka
Noriyuki Matsunaga
Yuji Ikeda
Hideyo Kawakita
Shogo Otsubo
Ayaka Watase
Daisuke Taniguchi
Misaki Mizumoto
Natsuko Izumi
Naoto Kobayashi
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Extinction law in ultraluminous infrared galaxies at z ~ 1
2011
arXiv: Cosmology and Nongalactic Astrophysics
T. Shimizu
Kimiaki Kawara
H. Sameshima
N. Ienaka
Takaya Nozawa
Takashi Kozasa
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Supernova dust for the extinction law in a young infrared galaxy at z = 1
2010
arXiv: Cosmology and Nongalactic Astrophysics
Kimiaki Kawara
Hiroyuki Hirashita
Takaya Nozawa
Takashi Kozasa
Shinki Oyabu
Yoshiki Matsuoka
T. Shimizu
H. Sameshima
N. Ienaka
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Stellar population and dust extinction in an ultraluminous infrared galaxy at z=1.135
2009
arXiv: Cosmology and Nongalactic Astrophysics
Kimiaki Kawara
Shinki Oyabu
Yoshiki Matsuoka
Yuzuru Yoshii
Takeo Minezaki
H. Sameshima
Naoko Asami
N. Ienaka
Takashi Kozasa
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