Zobrazeno 1 - 10
of 157
pro vyhledávání: '"Yano Taihei"'
Autor:
Kamizuka, Takafumi, Kawahara, Hajime, Ohsawa, Ryou, Kataza, Hirokazu, Kawata, Daisuke, Yamada, Yoshiyuki, Hirano, Teruyuki, Miyakawa, Kohei, Aizawa, Masataka, Omiya, Masashi, Yano, Taihei, Kano, Ryouhei, Wada, Takehiko, Löffler, Wolfgang, Biermann, Michael, Ramos, Pau, Isobe, Naoki, Usui, Fumihiko, Hattori, Kohei, Yoshioka, Satoshi, Tatekawa, Takayuki, Izumiura, Hideyuki, Fukui, Akihiko, Miyoshi, Makoto, Tatsumi, Daisuke, Gouda, Naoteru
Publikováno v:
Proc. SPIE, 13099, 130992D (2024)
JASMINE is a Japanese planned space mission that aims to reveal the formation history of our Galaxy and discover habitable exoEarths. For these objectives, the JASMINE satellite performs high-precision astrometric observations of the Galactic bulge a
Externí odkaz:
http://arxiv.org/abs/2410.03149
Autor:
Schoedel, Rainer, Longmore, Steve, Henshaw, Jonny, Ginsburg, Adam, Bally, John, Feldmeier, Anja, Hosek, Matt, Lara, Francisco Nogueras, Ciurlo, Anna, Chevance, Mélanie, Kruijssen, J. M. Diederik, Klessen, Ralf, Ponti, Gabriele, Amaro-Seoane, Pau, Anastasopoulou, Konstantina, Anderson, Jay, Arias, Maria, Barnes, Ashley T., Battersby, Cara, Bono, Giuseppe, Ferres, Lucía Bravo, Bryant, Aaron, Gonzáalez, Miguel Cano, Cassisi, Santi, Chaves-Velasquez, Leonardo, Conte, Francesco, Ramos, Rodrigo Contreras, Cotera, Angela, Crowe, Samuel, di Teodoro, Enrico, Do, Tuan, Eisenhauer, Frank, Enokiya, Rei, Fedriani, Rubén, Friske, Jennifer K. S., Gadotti, Dimitri, Gallart, Carme, Calvente, Teresa Gallego, Cano, Eulalia Gallego, Fuentes, Pablo García, Marín, Macarena García, Gardini, Angela, Gautam, Abhimat K., Ghez, Andrea, Gillessen, Stefan, Gouda, Naoteru, Gualandris, Alessia, Guarcello, Mario Giuseppe, Gutermuth, Robert, Haggard, Daryl, Hankins, Matthew, Hu, Yue, Kano, Ryohei, Kauffmann, Jens, Lau, Ryan, Lazarian, Alexandre, Libralato, Mattia, Lu, Anan, Lu, Xing, Lu, Jessica R., Luetzgendorf, Nora, Magorrian, John, Mandel, Shifra, Markoff, Sera, Arranz, Álvaro Martínez, Mastrobuono-Battisti, Alessandra, Melamed, Maria, Mills, Elisabeth, Mori, Kaya, Morris, Mark, Murchikova, Elena, Nagata, Tetsuya, Najarro, Francisco, Nandakumar, Govind, Nataf, David, Neumayer, Nadine, Nishiyama, Shogo, Nobukawa, Masayoshi, Paré, Dylan M, Peissker, Florian, Petkova, Maya, Pillai, Thushara G. S., Román, Mike Rich Carlos, Rugel, Michael, Ryde, Nils, Sabha, Nadeen, Bermúdez, Joel Sánchez, Sánchez-Monge, Álvaro, Schultheis, Mathias, Shao, Lijing, Shinnaga, Hiroko, Simpson, Janet, Takekawa, Shunya, Tan, Jonathan C., Thorsbro, Brian, Torne, Pablo, Tress, Robin Goppala, Uchiyam, Hideki, Valenti, Elena, van der Marel, Roeland, Verberne, Sill, Vermot, Pierre, von Fellenberg, Sebastiano, Walker, Daniel, Witzel, Gunther, Xu, Siyao, Yano, Taihei, Yusef-Zadeh, Farhad, Zajaček, Michal, Zoccali, Manuela
The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post main sequence stars, and the highest volume density of supernovae in the
Externí odkaz:
http://arxiv.org/abs/2310.11912
Autor:
Kawata, Daisuke, Kawahara, Hajime, Gouda, Naoteru, Secrest, Nathan J., Kano, Ryouhei, Kataza, Hirokazu, Isobe, Naoki, Ohsawa, Ryou, Usui, Fumihiko, Yamada, Yoshiyuki, Graham, Alister W., Pettitt, Alex R., Asada, Hideki, Baba, Junichi, Bekki, Kenji, Dorland, Bryan N., Fujii, Michiko, Fukui, Akihiko, Hattori, Kohei, Hirano, Teruyuki, Kamizuka, Takafumi, Kashima, Shingo, Kawanaka, Norita, Kawashima, Yui, Klioner, Sergei A., Kodama, Takanori, Koshimoto, Naoki, Kotani, Takayuki, Kuzuhara, Masayuki, Levine, Stephen E., Majewski, Steven R., Masuda, Kento, Matsunaga, Noriyuki, Miyakawa, Kohei, Miyoshi, Makoko, Morihana, Kumiko, Nishi, Ryoichi, Notsu, Yuta, Omiya, Masashi, Sanders, Jason, Tanikawa, Ataru, Tsujimoto, Masahiro, Yano, Taihei, Aizawa, Masataka, Arimatsu, Ko, Biermann, Michael, Boehm, Celine, Chiba, Masashi, Debattista, Victor P., Gerhard, Ortwin, Hirabayashi, Masayuki, Hobbs, David, Ikenoue, Bungo, Izumiura, Hideyuki, Jordi, Carme, Kohara, Naoki, Löffler, Wolfgang, Luri, Xavier, Mase, Ichiro, Miglio, Andrea, Mitsuda, Kazuhisa, Newswander, Trent, Nishiyama, Shogo, Obuchi, Yoshiyuki, Ootsubo, Takafumi, Ouchi, Masami, Ozaki, Masanobu, Perryman, Michael, Prusti, Timo, Ramos, Pau, Read, Justin I., Rich, R. Michael, Schönrich, Ralph, Shikauchi, Minori, Shimizu, Risa, Suematsu, Yoshinori, Tada, Shotaro, Takahashi, Aoi, Tatekawa, Takayuki, Tatsumi, Daisuke, Tsujimoto, Takuji, Tsuzuki, Toshihiro, Urakawa, Seitaro, Uraguchi, Fumihiro, Utsunomiya, Shin, Van Eylen, Vincent, van Leeuwen, Floor, Wada, Takehiko, Walton, Nicholas A.
Japan Astrometry Satellite Mission for INfrared Exploration (JASMINE) is a planned M-class science space mission by the Institute of Space and Astronautical Science, the Japan Aerospace Exploration Agency. JASMINE has two main science goals. One is t
Externí odkaz:
http://arxiv.org/abs/2307.05666
Autor:
Hattori, Kohei, Gouda, Naoteru, Yano, Taihei, Sakai, Nobuyuki, Tagawa, Hiromichi, Baba, Junichi, Kumamoto, Jun
The origin of the Hercules stream, the most prominent velocity substructure in the Solar neighbour disc stars, is still under debate. Recent accurate measurements of position, velocity, and metallicity provided by Tycho Gaia Astrometric Solution (TGA
Externí odkaz:
http://arxiv.org/abs/1804.01920
We investigate how accurately phase space distribution functions (DFs) in galactic models can be reconstructed by a made-to-measure (M2M) method, which constructs $N$-particle models of stellar systems from photometric and various kinematic data. The
Externí odkaz:
http://arxiv.org/abs/1608.04386
We perform numerical simulations on the merger of multiple black holes (BHs) in primordial gas at early cosmic epochs. We consider two cases of BH mass: $M_{BH} = 30 M_{\odot}$ and $M_{BH} = 10^4 M_{\odot}$. Attention is concentrated on the effect of
Externí odkaz:
http://arxiv.org/abs/1505.03151
Akademický článek
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A phase-space distribution function of the steady state in galaxy models that admits regular orbits overall in the phase-space can be represented by a function of three action variables. This type of distribution function in Galactic models is often
Externí odkaz:
http://arxiv.org/abs/1405.2393
Autor:
Egner, Sébastien E., Roberts, Scott, Kamizuka, Takafumi, Kawahara, Hajime, Ohsawa, Ryou, Kataza, Hirokazu, Kawata, Daisuke, Yamada, Yoshiyuki, Hirano, Teruyuki, Miyakawa, Kohei, Aizawa, Masataka, Omiya, Masashi, Yano, Taihei, Kano, Ryouhei, Wada, Takehiko, Löffler, Wolfgang, Biermann, Michael, Ramos, Pau, Isobe, Naoki, Usui, Fumihiko, Hattori, Kohei, Yoshioka, Satoshi, Tatekawa, Takayuki, Izumiura, Hideyuki, Fukui, Akihiko, Miyoshi, Makoto, Tatsumi, Daisuke, Gouda, Naoteru
Publikováno v:
Proceedings of SPIE; September 2024, Vol. 13099 Issue: 1 p130992D-130992D-13, 12968222p
Autor:
Coyle, Laura E., Matsuura, Shuji, Perrin, Marshall D., Kataza, Hirokazu, Kano, Ryouhei, Gouda, Naoteru, Hirabayashi, Masayuki, Isobe, Naoki, Kamizuka, Takafumi, Kashima, Shingo, Kawahara, Hajime, Kawata, Daisuke, Kohara, Naoki, Kondo, Iona, Mase, Ichiro, Miyakawa, Kohei, Ohsawa, Ryou, Ozaki, Masanobu, Shimizu, Risa, Suematsu, Yoshinori, Tada, Shotaro, Tsuzuki, Toshihiro, Uraguchi, Fumihiro, Usui, Fumihiko, Utsunomiya, Shin, Wada, Takehiko, Yamada, Yoshiyuki, Yano, Taihei
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13092 Issue: 1 p130920A-130920A-9, 1178290p