Zobrazeno 1 - 10
of 13
pro vyhledávání: '"M. W. McElwain"'
Autor:
Edwin L. Turner, M. W. McElwain, Th. Henning, Takuya Suenaga, Taro Matsuo, Toru Yamada, Makoto Watanabe, John P. Wisniewski, Takayuki Kotani, Tae-Soo Pyo, Olivier Guyon, Jennifer L. Karr, Masanori Iye, Y. Maruta, Yasuhiro H. Takahashi, Joseph C. Carson, Michihiro Takami, Takayuki Muto, Nobuhiko Kusakabe, Miwa Goto, M. Feldt, R. Suzuki, Naruhisa Takato, C. Thalmann, Yoshiko K. Okamoto, Mickael Bonnefoy, Hiroshi Suto, D. Tomono, Jun Hashimoto, Amaya Moro-Martin, Carol A. Grady, Hiroshi Terada, Timothy D. Brandt, Motohide Tamura, Markus Janson, Eugene Serabyn, R. Kandori, Masahiko Hayashi, Jun-Ichi Morino, Masayuki Kuzuhara, Misato Fukagawa, Shoken Miyama, Sebastian Egner, Saeko S. Hayashi, Munetake Momose, Jungmi Kwon, Tetsuo Nishimura, Miki Ishii, Tomoyuki Kudo, Katherine B. Follette, Lyu Abe, Hideki Takami, Gillian R. Knapp, T. Currie, Klaus W. Hodapp, Y. Ohta, Michael L. Sitko, Wolfgang Brandner, Yutaka Hayano, Tomonori Usuda
Publikováno v:
Astrophysics and Space Science. 355:253-266
Spatially-resolved imaging of Herbig stars and related objects began with HST, but intensified with commissioning of high-contrast imagers on 8-m class telescopes. The bulk of the data taken from the ground have been polarized intensity imagery at H-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b0700be3e1df5a546c4b68307bdc65e7
https://doi.org/10.1007/s10509-014-2214-2
https://doi.org/10.1007/s10509-014-2214-2
Autor:
M. W. McElwain, Ben Placek, Matthias Mallonn, Eric E. Becklin, Edward W. Dunham, P. Collins, S. Shenoy, C. Dreyer, Daniel Kitzmann, Enrico Pfueller, Avi Mandell, M. Godolt, J. Van Cleve, Petr Kabath, Sarah E. Logsdon, Ph. Eigmüller, Ian S. McLean, Jürgen Wolf, Daniel Angerhausen, Heike Rauer, G. Mandushev, Ryan T. Hamilton, William D. Vacca, M. Savage, John Lee Grenfell, Sz. Csizmadia, Manuel Wiedemann
The benchmark exoplanet GJ 1214b is one of the best studied transiting planets in the transition zone between rocky Earth-sized planets and gas or ice giants. This class of super-Earth/mini-Neptune planets is unknown in our Solar System, yet is one o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae457515674e5a9c016bcea3fbd3f6b9
https://doi.org/10.1051/0004-6361/201730914
https://doi.org/10.1051/0004-6361/201730914
Autor:
Saeko S. Hayashi, Takayuki Muto, M. Feldt, Miwa Goto, Jennifer I-Hsiu Li, Tetsuo Nishimura, Hideki Takami, Th. Henning, Motohide Tamura, Ryo Kandori, Takuya Suenaga, Yutaka Hayano, M. L. Sitko, Hiroshi Terada, Tetsuo Taki, M. Bonnefoy, M. Hayashi, Hauyu Baobabu Liu, Nagayoshi Ohashi, Shoken M. Miyama, Gillian R. Knapp, M. W. McElwain, Sebastian Egner, Ruobing Dong, Tomonori Usuda, Timothy D. Brandt, Tae-Soo Pyo, Eugene Serabyn, Olivier Guyon, Tomoyuki Kudo, Makoto Watanabe, John P. Wisniewski, Eiji Akiyama, Taro Matsuo, D. Tomono, Markus Janson, Miki Ishii, T. Tsukagoshi, Munetake Momose, C. A. Grady, Masayuki Kuzuhara, Wolfgang Brandner, Amaya Moro-Martin, Yasuhiro Hasegawa, Lyu Abe, Jungmi Kwon, Masanori Iye, Joseph C. Carson, Klaus W. Hodapp, Hiroshi Suto, Edwin L. Turner, Y. H. Takahashi, Jun-Ichi Morino, Jun Hashimoto, Satoshi Mayama, N. Kusakabe, Naruhisa Takato, C. Thalmann, Michihiro Takami, R. Suzuki, Toru Yamada
Publikováno v:
NASA Astrophysics Data System
Dust trapping accelerates the coagulation of dust particles, and thus it represents an initial step toward the formation of planetesimals. We report $H$-band (1.6 um) linear polarimetric observations and 0.87 mm interferometric continuum observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::06f8b6dfe5194df63590ee43a28f8f7e
http://arxiv.org/abs/1607.04708
http://arxiv.org/abs/1607.04708
Autor:
Masayuki Kuzuhara, Misato Fukagawa, Shoken Miyama, Ryo Kandori, Amaya Moro-Martin, Thomas Henning, Joseph C. Carson, Klaus W. Hodapp, Hideki Takami, M. W. McElwain, Carol A. Grady, Sebastian Egner, Yutaka Hayano, John P. Wisniewski, Timothy D. Brandt, Takahiro Sumi, Mihoko Konishi, Jun-Ichi Morino, Ryuji Suzuki, Eugene Serabyn, Yoichi Itoh, Ryoko Tanii, Miwa Goto, Nobuhiko Kusakabe, J. Nishikawa, Taro Matsuo, Saeko S. Hayashi, Masanori Iye, Motohide Tamura, Jun Sudo, Toru Yamada, Christian Thalmann, Naruhisa Takato, Lyu Abe, Masahiko Hayashi, Gillian R. Knapp, Kodai Yamamoto, Edwin Lewis Turner, Markus Feldt, Markus Janson, Miki Ishii, Tomonori Usuda, Tomoyuki Kudo, Makoto Watanabe, Tae-Soo Pyo, Jun Hashimoto, Olivier Guyon, Wolfgang Brandner, Hiroshi Shibai, Jungmi Kwon, Daigo Tomono, Thayne Currie, Hiroshi Terada, Michihiro Takami, Tetsuo Nishimura, Hiroshi Suto
Publikováno v:
Publications of the Astronomical Society of Japan, 65(4):90. Astronomical Society of Japan
Scopus-Elsevier
Scopus-Elsevier
We carried out an imaging survey for extrasolar planets around stars in the Pleiades (125 Myr, 135 pc) in the $H$ and $K_{S}$ bands using HiCIAO combined with the adaptive optics, AO188, on the Subaru telescope. We found 13 companion candidates faint
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a9c8c7d64750fc1aa52dfffcba7039b
https://doi.org/10.1093/pasj/65.4.90
https://doi.org/10.1093/pasj/65.4.90
Autor:
Takao Nakagawa, Hideki Takami, Saeko S. Hayashi, Naruhisa Takato, C. Thalmann, Gillian R. Knapp, Th. Henning, Amaya Moro-Martin, Takuya Suenaga, Jungmi Kwon, Ryo Kandori, Masayuki Kuzuhara, Tetsuro Nishimura, Yutaka Hayano, Edwin L. Turner, M. W. McElwain, Tomoyuki Kudo, Shoken Miyama, Lyu Abe, Tomonori Usuda, Michael L. Sitko, Eugene Serabyn, Hiroshi Terada, Miki Ishii, Motohide Tamura, Masanori Iye, Michihiro Takami, Joseph C. Carson, Taro Matsuo, Carol A. Grady, R. Suzuki, W. Brander, J. Nishikawa, Hiroshi Suto, Toshiyuki Mizuki, Jun-Ichi Morino, Jun Hashimoto, Toru Yamada, Tae-Soo Pyo, N. Kusakabe, Olivier Guyon, Yasuhiro H. Takahashi, Markus Janson, Sebastian Egner, Klaus W. Hodapp, M. Hayashi, Makoto Watanabe, Timothy D. Brandt, M. Feldt, Miwa Goto, John P. Wisniewski
Publikováno v:
Astronomy & Astrophysics. 595:A79
epsilon Eridani is one of the nearest solar-type stars. Its proximity and relatively young age allow high-contrast imaging observations to achieve sensitivities to planets at narrow separations down to an inner radius of similar to 5 AU. Previous obs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::330805e10f3369cad35bb2f013db3419
https://doi.org/10.1051/0004-6361/201628544
https://doi.org/10.1051/0004-6361/201628544
Autor:
N. Kusakabe, C. A. Grady, M. L. Sitko, J. Hashimoto, T. Kudo, M. Fukagawa, T. Muto, J. P. Wisniewski, M. Min, S. Mayama, C. Werren, A. N. Day, L. C. Beerman, D. K. Lynch, R. W. Russell, S. M. Brafford, M. Kuzuhara, T. D. Brandt, L. Abe, W. Brandner, J. Carson, S. Egner, M. Feldt, M. Goto, O. Guyon, Y. Hayano, M. Hayashi, S. S. Hayashi, T. Henning, K. W. Hodapp, M. Ishii, M. Iye, M. Janson, R. Kandori, G. R. Knapp, T. Matsuo, M. W. McElwain, S. Miyama, J.-I. Morino, A. Moro-Martin, T. Nishimura, T.-S. Pyo, H. Suto, R. Suzuki, M. Takami, N. Takato, H. Terada, C. Thalmann, D. Tomono, E. L. Turner, M. Watanabe, T. Yamada, H. Takami, T. Usuda, M. Tamura
Publikováno v:
Astrophysical Journal, 753(2). IOP Publishing Ltd.
One of the key predictions of modeling from the IR excess of Herbig Ae stars is that for protoplanetary disks, where significant grain growth and settling has occurred, the dust disk has flattened to the point that it can be partially or largely shad
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ac9070ac8d5aebc4a7927533c3829389
https://doi.org/10.1088/0004-637x/753/2/153
https://doi.org/10.1088/0004-637x/753/2/153
Autor:
M. W. McElwain, Yutaka Hayano, Tetsuro Nishimura, Gillian R. Knapp, Yasuhiro H. Takahashi, Tomoyuki Kudo, C. A. Grady, Tae-Soo Pyo, Takashi Tsukagoshi, Jungmi Kwon, Th. Henning, Shoken Miyama, Olivier Guyon, Takuya Suenaga, Markus Janson, Hideki Takami, Ryo Kandori, M. Ishi, Jun Hashimoto, Edwin L. Turner, Lyu Abe, Masanori Iye, Satoshi Mayama, Tomonori Usuda, Eiji Akiyama, Joseph C. Carson, Timothy D. Brandt, Naruhisa Takato, C. Thalmann, John P. Wisniewski, Hiroshi Terada, Thayne Currie, Taro Matsuo, Klaus W. Hodapp, Michihiro Takami, Hiroshi Suto, Amaya Moro-Martin, Nobuhiko Kusakabe, R. Suzuki, Saeko S. Hayashi, Masayuki Kuzuhara, Akimasa Kataoka, Jun-Ichi Morino, Toru Yamada, Miwa Goto, Motohide Tamura, Masahiko Hayashi, Wolfgang Brandner, Munetake Momose, Sebastian Egner, Nagayoshi Ohashi, Makoto Watanabe, Michael L. Sitko, D. Tomono, Takayuki Muto, M. Feldt, G. Serabyn
Publikováno v:
The Astrophysical Journal. 802:L17
We present a new Subaru/HiCIAO high-contrast H-band polarized intensity (PI) image of a nearby transitional disk associated with TW Hydrae. The scattered light from the disk was detected from 0.2" to 1.5" (11 - 81 AU) and the PI image shows a clear a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f3c775d1fc029475d0a8be3e5b642c6f
https://doi.org/10.1088/2041-8205/802/2/l17
https://doi.org/10.1088/2041-8205/802/2/l17
Autor:
Tomonori Usuda, Masayuki Kuzuhara, Hiroshi Suto, David J. Wilner, Joseph C. Carson, Carol A. Grady, Miki Ishii, Ryo Kandori, Klaus W. Hodapp, Miwa Goto, Yutaka Hayano, Saeko S. Hayashi, Munetake Momose, M. W. McElwain, Yasuhiro H. Takahashi, Masanori Iye, Ryuji Suzuki, Tae-Soo Pyo, Timothy D. Brandt, Ryohei Kawabe, Hiroshi Terada, Olivier Guyon, Edwin L. Turner, Hideki Takami, Naruhisa Takato, Tetsuro Nishimura, Taro Matsuo, Takashi Tsukagoshi, Motohide Tamura, Takuya Suenaga, Markus Janson, Toru Yamada, Yoshimi Kitamura, Eugene Serabyn, Masahiko Hayashi, Tomoyuki Kudo, Eiji Akiyama, Gillian R. Knapp, Jun-Ichi Morino, Nobuhiko Kusakabe, Jun Hashimoto, Amaya Moro-Martin, Michihiro Takami, Wolfgang Brandner, John P. Wisniewski, Sean M. Andrews, Satoshi Mayama, Masao Saito, Jungmi Kwon, Lyu Abe, Thayne Currie, Shoken Miyama, Thomas Henning, Sebastian Egner, Nagayoshi Ohashi, Christian Thalmann, Makoto Watanabe, Daigo Tomono
Publikováno v:
Astrophysical Journal, 783(2). IOP Publishing Ltd.
著者人数: 58名
Accepted: 2014-01-16
資料番号: SA1004554000
Accepted: 2014-01-16
資料番号: SA1004554000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::212b75d3181bac90dc90a2309eebeb29
https://dare.uva.nl/personal/pure/en/publications/highresolution-submillimeter-and-nearinfrared-studies-of-the-transition-disk-around-sz-91(7c85e66a-5636-445e-9684-36e3abebacc1).html
https://dare.uva.nl/personal/pure/en/publications/highresolution-submillimeter-and-nearinfrared-studies-of-the-transition-disk-around-sz-91(7c85e66a-5636-445e-9684-36e3abebacc1).html
Autor:
Makoto Watanabe, D. Tomono, Th. Henning, Takuya Suenaga, N. Kusakabe, M. W. McElwain, Sebastian Egner, M. Hayashi, Jungmi Kwon, Hiroshi Terada, Yutaka Hayano, Ryo Kandori, Markus Janson, Jun-Ichi Morino, Michihiro Takami, Takayuki Muto, Tae-Soo Pyo, G. Serabyn, M. Feldt, Olivier Guyon, R. Suzuki, Hideki Takami, Tomonori Usuda, Toru Yamada, Taro Matsuo, Motohide Tamura, Tetsuro Nishimura, Misato Fukagawa, Tomoyuki Kudo, Shoken Miyama, Jun Hashimoto, Amaya Moro-Martin, John P. Wisniewski, Timothy D. Brandt, Saeko S. Hayashi, Masayuki Kuzuhara, Miwa Goto, Christian Thalmann, Klaus W. Hodapp, Gillian R. Knapp, Zhaohuan Zhu, Lyu Abe, M. K. McClure, Masanori Iye, Joseph C. Carson, Ruobing Dong, Hiroshi Suto, Wolfgang Brandner, Naruhisa Takato, Edwin L. Turner, Yasuhiro H. Takahashi, Satoshi Mayama, Mitsuhiko Honda, Carol A. Grady, Miki Ishii
Publikováno v:
The Astrophysical Journal. 775:L33
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ce0fd65cdbe091c8e29404ef45347e43
https://doi.org/10.1088/2041-8205/775/1/l33
https://doi.org/10.1088/2041-8205/775/1/l33
Autor:
T. Mizuki, M. Kuzuhara, K. Mede, J. E. Schlieder, M. Janson, T. D. Brandt, T. Hirano, N. Narita, J. Wisniewski, T. Yamada, B. Biller, M. Bonnefoy, J. C. Carson, M. W. McElwain, T. Matsuo, E. L. Turner, S. Mayama, E. Akiyama, T. Uyama, T. Nakagawa
Publikováno v:
Astrophysical Journal; 10/1/2018, Vol. 865 Issue 2, p1-1, 1p