Zobrazeno 1 - 10
of 254
pro vyhledávání: '"Kandori, Ryo"'
Autor:
Lomax, Jamie R., Wisniewski, John P., Grady, Carol A., McElwain, Michael W., Hashimoto, Jun, Kudo, Tomoyuki, Kusakabe, Nobuhiko, Okamoto, Yoshiko K., Fukagawa, Misato, Abe, Lyu, Brandner, Wolfgang, Brandt, Timothy D., Carson, Joseph C., Currie, Thayne M, Egner, Sebastian, Feldt, Markus, Goto, Miwa, Guyon, Olivier, Hayano, Yutaka, Hayashi, Masahiko, Hayashi, Saeko S., Henning, Thomas, Hodapp, Klaus W., Inoue, Akio, Ishii, Miki, Iye, Masanori, Janson, Markus, Kandori, Ryo, Knapp, Gillian R., Kuzuhara, Masayuki, Kwon, Jungmi, Matsuo, Taro, Mayama, Satoshi, Miyama, Shoken, Momose, Munetake, Morino, Jun-Ichi, Moro-Martin, Amaya, Nishimura, Tetsuo, Pyo, Tae-Soo, Schneider, Glenn H, Serabyn, Eugene, Sitko, Michael L., Suenaga, Takuya, Suto, Hiroshi, Suzuki, Ryuji, Takahashi, Yasuhiro H., Takami, Michihiro, Takato, Naruhisa, Terada, Hiroshi, Thalmann, Christian, Tomono, Daigo, Turner, Edwin L., Watanabe, Makoto, Yamada, Toru, Takami, Hideki, Usuda, Tomonori, Tamura, Motohide
We present a new analysis of multi-epoch, H-band, scattered light images of the AB Aur system. We use a Monte Carlo radiative transfer code to simultaneously model the system's spectral energy distribution (SED) and H-band polarized intensity (PI) im
Externí odkaz:
http://hdl.handle.net/10150/622048
http://arizona.openrepository.com/arizona/handle/10150/622048
http://arizona.openrepository.com/arizona/handle/10150/622048
Autor:
Tatematsu, Ken'ichi, Yeh, You-Ting, Hirano, Naomi, Liu, Sheng-Yuan, Liu, Tie, Dutta, Somnath, Sahu, Dipen, Evans II, Neal J., Juvela, Mika, Yi, Hee-Weon, Lee, Jeong-Eun, Sanhueza, Patricio, Li, Shanghuo, Eden, David, Kim, Gwanjeong, Lee, Chin-Fei, Wu, Yuefang, Kim, Kee-Tae, T'oth, L. Viktor, Choi, Minho, Kang, Miju, Thompson, Mark A., Fuller, Gary A., Di Li, 20, Wang, Ke, Sakai, Takeshi, Kandori, Ryo, Hsu, Shih-Ying, Chiong, Chau-Ching, collaboration, JCMT Large Program SCOPE, collaboration, ALMASOP
Publikováno v:
Astrophysical J. 931 (2022) 33
In this study, 36 cores (30 starless and 6 protostellar) identified in Orion were surveyed to search for inward motions. We used the Nobeyama 45 m radio telescope, and mapped the cores in the $J = 1\rightarrow0$ transitions of HCO$^+$, H$^{13}$CO$^+$
Externí odkaz:
http://arxiv.org/abs/2203.12885
Autor:
Tatematsu, Ken'ichi, Kim, Gwanjeong, Liu, Tie, Evans II, Neal J., Yi, Hee-Weon, Lee, Jeong-Eun, Wu, Yuefang, Hirano, Naomi, Liu, Sheng-Yuan, Dutta, Somnath, Sahu, Dipen, Sanhueza, Patricio, Kim, Kee-Tae, Juvela, Mika, T'oth, L. Viktor, Feh'er, Orsolya, He, Jinhua, Ge, J. X., Feng, Siyi, Choi, Minho, Kang, Miju, Thompson, Mark A., Fuller, Gary A., Li, Di, Ristorcelli, Isabelle, Wang, Ke, Di Francesco, James, Eden, David, Ohashi, Satoshi, Kandori, Ryo, Vastel, Charlotte, Hirota, Tomoya, Sakai, Takeshi, Lu, Xing, Lu'o'ng, Quang Nguyen, Shinnaga, Hiroko, Kim, Jungha, collaboration, JCMT Large Program "SCOPE''
Publikováno v:
Astrophys.J.Suppl. 256 (2021) 25
We present the results of on-the-fly mapping observations of 44 fields containing 107 SCUBA-2 cores in the emission lines of molecules, N$_2$H$^+$, HC$_3$N, and CCS at 82$-$94 GHz using the Nobeyama 45-m telescope. This study aimed at investigating t
Externí odkaz:
http://arxiv.org/abs/2106.04052
Autor:
Kandori, Ryo, Tamura, Motohide, Saito, Masao, Tomisaka, Kohji, Matsumoto, Tomoaki, Tazaki, Ryo, Nagata, Tetsuya, Kusakabe, Nobuhiko, Nakajima, Yasushi, Kwon, Jungmi, Nagayama, Takahiro, Tatematsu, Ken'ichi
Detailed magnetic field structure of the dense core SL42 (CrA-E) in the Corona Australis molecular cloud complex was investigated based on near-infrared polarimetric observations of background stars to measure dichroically polarized light produced by
Externí odkaz:
http://arxiv.org/abs/2007.15436
Autor:
Kim, Gwanjeong, Tatematsu, Kenichi, Liu, Tie, Yi, Miss Hee-Weon, He, Jinhua, Hirano, Naomi, Liu, Sheng-Yuan, Choi, Minho, Sanhueza, Patricio, Toth, L. Viktor, Evans, Neal J., Feng, Siyi, Juvela, Mika, Kim, Kee-Tae, Vastel, Charlotte, Lee, Jeong-Eun, Nguyn-Lu'o'ng, Quang, Kang, Miju, Ristorcelli, Isabelle, Fehér, O., Wu, Yuefang, Ohashi, Satoshi, Wang, Ke, Kandori, Ryo, Hirota, Tomoya, Sakai, Takeshi, Lu, Xing, Thompson, Mark A., Fuller, Gary A., Li, Di, Shinnaga, Hiroko, Kim, Jungha
We present the results of a single-pointing survey of 207 dense cores embedded in Planck Galactic Cold Clumps distributed in five different environments ($\lambda$ Orionis, Orion A, B, Galactic plane, and high latitudes) to identify dense cores on th
Externí odkaz:
http://arxiv.org/abs/2007.12319
Autor:
Tatematsu, Ken'ichi, Liu, Tie, Kim, Gwanjeong, Yi, Hee-Weon, Lee, Jeong-Eun, Hirano, Naomi, Liu, Sheng-Yuan, Ohashi, Satoshi, Sanhueza, Patricio, Di Francesco, James, Evans II, Neal J., Fuller, Gary A., Kandori, Ryo, Choi, Minho, Kang, Miju, Feng, Siyi, Hirota, Tomoya, Sakai, Takeshi, Lu, Xing, Lu'o'ng, Quang Nguyen, Thompson, Mark A., Wu, Yuefang, Li, Di, Kim, Kee-Tae, Wang, Ke, Ristorcelli, Isabelle, Juvela, Mika, T'oth, L. Viktor
Publikováno v:
Astrophys.J. 895 (2020) 119
We mapped two molecular cloud cores in the Orion A cloud with the ALMA ACA 7-m Array and with the Nobeyama 45-m radio telescope. These cores have bright N$_2$D$^+$ emission in single-pointing observations with the Nobeyama 45-m radio telescope, have
Externí odkaz:
http://arxiv.org/abs/2004.12548
Autor:
Hirao, Yuki, Bennett, David P., Ryu, Yoon-Hyun, Koshimoto, Naoki, Udalski, Andrzej, Yee, Jennifer C., Sumi, Takahiro, Bond, Ian A., Shvartzvald, Yossi, Abe, Fumio, Barry, Richard K., Bhattacharya, Aparna, Donachie, Martin, Fukui, Akihiko, Itow, Yoshitaka, Kondo, Iona, Li, Man Cheung Alex, Matsubara, Yutaka, Matsuo, Taro, Miyazaki, Shota, Muraki, Yasushi, Nagakane, Masayuki, Ranc, Clement, Rattenbury, Nicholas J., Suematsu, Haruno, Shibai, Hiroshi, Suzuki, Daisuke, Tristram, Paul J., Yonehara, Atsunori, Skowron, J., Poleski, R., Mroz, P., Szymanski, M. K., Soszynski, I., Kozlowski, S., Pietrukowicz, P., Ulaczyk, K., Rybicki, K., Iwanek, P., Albrow, Michael D., Chung, Sun-Ju, Gould, Andrew, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, Shin, In-Gu, Zang, Weicheng, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Hyoun-Woo, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Beichman, Charles A., Bryden, Geoffery, Novati, Sebastiano Calchi, Carey, Sean, Gaudi, B. Scott, Henderson, Calen B., Zhu, Wei, Bachelet, Etienne, Bolt, Greg, Christie, Grant, Hundertmark, Markus, Natusch, Tim, Maoz, Dan, McCormick, Jennie, Street, Rachel A., Tan, Thiam-Guan, Tsapras, Yiannis, Jorgensen, U. G., Dominik, M., Bozza, V., Skottfelt, J., Snodgrass, C., Ciceri, S., Jaimes, R. Figuera, Evans, D. F., Peixinho, N., Hinse, T. C., Burgdorf, M. J., Southworth, J., Rahvar, S., Sajadian, S., Rabus, M., von Essen, C., Fujii, Y. I., Campbell-White, J., Lowry, S., Helling, C., Mancini, L., Haikala, L., Kandori, Ryo
We report the discovery and analysis of the planetary microlensing event OGLE-2017-BLG-0406, which was observed both from the ground and by the ${\it Spitzer}$ satellite in a solar orbit. At high magnification, the anomaly in the light curve was dens
Externí odkaz:
http://arxiv.org/abs/2004.09067
Autor:
Kandori, Ryo, Tamura, Motohide, Saito, Masao, Tomisaka, Kohji, Matsumoto, Tomoaki, Tazaki, Ryo, Nagata, Tetsuya, Kusakabe, Nobuhiko, Nakajima, Yasushi, Kwon, Jungmi, Nagayama, Takahiro, Tatematsu, Ken'ichi
The magnetic field structure of a star-forming Bok globule BHR 71 was determined based on near-infrared polarimetric observations of background stars. The magnetic field in BHR 71 was mapped from 25 stars. By using a simple 2D parabolic function, the
Externí odkaz:
http://arxiv.org/abs/2002.12512
Autor:
Kandori, Ryo, Saito, Masao, Tamura, Motohide, Tomisaka, Kohji, Matsumoto, Tomoaki, Tazaki, Ryo, Nagata, Tetsuya, Kusakabe, Nobuhiko, Nakajima, Yasushi, Kwon, Jungmi, Nagayama, Takahiro, Tatematsu, Ken'ichi
In this study, the detailed magnetic field structure of the dense protostellar core Barnard 335 (B335) was revealed based on near-infrared polarimetric observations of background stars to measure dichroically polarized light produced by magnetically
Externí odkaz:
http://arxiv.org/abs/2001.08542
Autor:
Yang, Yi, Akiyama, Eiji, Currie, Thayne, Dong, Ruobing, Hashimoto, Jun, Hayashi, Saeko S., Grady, Carol A., Janson, Markus, Jovanovic, Nemanja, Uyama, Taichi, Nakagawa, Takao, Kudo, Tomoyuki, Kusakabe, Nobuhiko, Kuzuhara, Masayuki, Abe, Lyu, Brandner, Wolfgang, Brandt, Timothy D., Bonnefoy, Michael, Carson, Joseph C., Chilcote, Jeffrey, Rich, Evan A., Feldt, Markus, Goto, Miwa, Groff, Tyler, Guyon, Olivier, Hayano, Yutaka, Hayashi, Masahiko, Henning, Thomas, Hodapp, Klaus W., Ishii, Miki, Iye, Masanori, Kandori, Ryo, Kasdin, Jeremy, Knapp, Gillian R., Kwon, Jungmi, Lozi, Julien, Martinache, Frantz, Matsuo, Taro, Mayama, Satoshi, Mcelwain, Michael W., Miyama, Shoken, Morino, Jun-Ichi, Moro-Martin, Amaya, Nishimura, Tetsuo, Pyo, Tae-Soo, Serabyn, Eugene, Suto, Hiroshi, Suzuki, Ryuji, Takami, Michihiro, Takato, Naruhisa, Terada, Hiroshi, Thalmann, Christian, Turner, Edwin L., Watanabe, Makoto, Wisniewski, John P., Yamada, Toru, Takami, Hideki, Usuda, Tomonori, Tamura, Motohide
We analyzed the young (2.8-Myr-old) binary system FS Tau A using near-infrared (H-band) high-contrast polarimetry data from Subaru/HiCIAO and sub-millimeter CO (J=2-1) line emission data from ALMA. Both the near-infrared and sub-millimeter observatio
Externí odkaz:
http://arxiv.org/abs/1912.11301