Zobrazeno 1 - 10
of 186
pro vyhledávání: '"Satoshi, Ohashi"'
Autor:
Ziwei E. Zhang, Nami Sakai, Satoshi Ohashi, Nadia M. Murillo, Claire J. Chandler, Brian Svoboda, Cecilia Ceccarelli, Claudio Codella, Luca Cacciapuoti, Ross O’Donoghue, Serena Viti, Yuri Aikawa, Eleonora Bianchi, Paola Caselli, Steven Charnley, Tomoyuki Hanawa, Izaskun Jímenez-Serra, Hauyu Baobab Liu, Laurent Loinard, Yoko Oya, Linda Podio, Giovanni Sabatini, Charlotte Vastel, Satoshi Yamamoto
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 2, p 207 (2024)
IRAS04368+2557 in L1527 is a Class 0/I protostar with a clear disk-envelope system revealed by previous Atacama Large Millimeter/submillimeter Array (ALMA) observations. In this paper, we discuss the flared structure of this source with observed sulf
Externí odkaz:
https://doaj.org/article/1b503ce7004a46b19788c0bb1bd2bb8c
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 2, p 190 (2023)
Embedded class 0/I protostellar disks represent the initial condition for planet formation. This calls for a better understanding of their bulk properties and the dust grains within them. We model multiwavelength dust continuum observations of the di
Externí odkaz:
https://doaj.org/article/c78a284d67564b0594545a6edc6761ac
Autor:
Satoshi Ohashi, Munetake Momose, Akimasa Kataoka, Aya E Higuchi, Takashi Tsukagoshi, Takahiro Ueda, Claudio Codella, Linda Podio, Tomoyuki Hanawa, Nami Sakai, Hiroshi Kobayashi, Satoshi Okuzumi, Hidekazu Tanaka
Publikováno v:
The Astrophysical Journal, Vol 954, Iss 2, p 110 (2023)
Characterizing the physical properties of dust grains in a protoplanetary disk is critical to comprehending the planet formation process. Our study presents Atacama Large Millimeter/submillimeter Array (ALMA) high-resolution observations of the young
Externí odkaz:
https://doaj.org/article/7ea2171308bb47aeb1cb9b4c11a8bbd4
Autor:
Ziwei E. Zhang, Yao-lun Yang, Yichen Zhang, Erin G. Cox, Shaoshan Zeng, Nadia M. Murillo, Satoshi Ohashi, Nami Sakai
Publikováno v:
The Astrophysical Journal, Vol 946, Iss 2, p 113 (2023)
In protostellar cores, sulfur species are effective probes for the energetic environments, such as shocked regions. With the majority of sulfur depleted on dust grains, sulfur-bearing molecules could be liberated back to gas phase by shocks associate
Externí odkaz:
https://doaj.org/article/0bcc380f81f848fba66dd57096ff5fdb
Autor:
Yukinori Sakata, Toshiyuki Matsuoka, Satoshi Ohashi, Tadashi Koga, Tetsumi Toyoda, Mika Ishii
Publikováno v:
Drugs - Real World Outcomes, Vol 6, Iss 1, Pp 27-35 (2019)
Abstract Background To understand the extent to which a large-scale healthcare claims database (DB) captures the safety profile of eribulin mesylate (Halaven®, Eisai Co., Ltd., Japan), we compared patient characteristics, drug use, and adverse event
Externí odkaz:
https://doaj.org/article/b6e8343596d0485190aac91691143bbc
Publikováno v:
Sensors, Vol 22, Iss 9, p 3296 (2022)
This study examined competitive wheelchairs that facilitate sports participation. They can be moved straight ahead using only one arm. Our designed and developed competitive wheel-chairs have a dual hand-rim system. Their two hand-rims, attached to a
Externí odkaz:
https://doaj.org/article/df61370d46434fd383dc285724270e7a
For revealing the first step of the plant formation, it is important to understand how and when dust grains become larger in a disk around a protostar. To investigate the grain growth, we analyze dust continuum emission toward a disk around the Class
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f3296667cdccab0aaa8306e8fa9fdbf2
http://arxiv.org/abs/2206.07800
http://arxiv.org/abs/2206.07800
Publikováno v:
International Sports Engineering Association – Engineering of Sport
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::895f4ccc3a504fc62151dd13a971c545
https://docs.lib.purdue.edu/resec-isea/2022/posters/15
https://docs.lib.purdue.edu/resec-isea/2022/posters/15
Autor:
Muneaki Imai, Yoko Oya, Brian Svoboda, Hauyu Baobab Liu, Bertrand Lefloch, Serena Viti, Yichen Zhang, Cecilia Ceccarelli, Claudio Codella, Claire J. Chandler, Nami Sakai, Yuri Aikawa, Felipe O. Alves, Nadia Balucani, Eleonora Bianchi, Mathilde Bouvier, Gemma Busquet, Paola Caselli, Emmanuel Caux, Steven Charnley, Spandan Choudhury, Nicolas Cuello, Marta De Simone, Francois Dulieu, Aurora Durán, Lucy Evans, Cécile Favre, Davide Fedele, Siyi Feng, Francesco Fontani, Logan Francis, Tetsuya Hama, Tomoyuki Hanawa, Eric Herbst, Shingo Hirano, Tomoya Hirota, Andrea Isella, Izaskun Jímenez-Serra, Doug Johnstone, Claudine Kahane, Romane Le Gal, Laurent Loinard, Ana López-Sepulcre, Luke T. Maud, María José Maureira, Francois Menard, Seyma Mercimek, Anna Miotello, George Moellenbrock, Shoji Mori, Nadia M. Murillo, Riouhei Nakatani, Hideko Nomura, Yasuhiro Oba, Ross O’Donoghue, Satoshi Ohashi, Yuki Okoda, Juan Ospina-Zamudio, Jaime Pineda, Linda Podio, Albert Rimola, Takeshi Sakai, Dominique Segura-Cox, Yancy Shirley, Vianney Taquet, Leonardo Testi, Charlotte Vastel, Naoki Watanabe, Yoshimasa Watanabe, Arezu Witzel, Ci Xue, Bo Zhao, Satoshi Yamamoto
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, 2022, 934 (1), pp.70. ⟨10.3847/1538-4357/ac77e7⟩
The Astrophysical Journal, 934(1):70
The Astrophysical Journal, 2022, 934 (1), pp.70. ⟨10.3847/1538-4357/ac77e7⟩
The Astrophysical Journal, 934(1):70
Imai et al.
The chemical diversity of low-mass protostellar sources has so far been recognized, and environmental effects are invoked as its origin. In this context, observations of isolated protostellar sources without the influence of nearby o
The chemical diversity of low-mass protostellar sources has so far been recognized, and environmental effects are invoked as its origin. In this context, observations of isolated protostellar sources without the influence of nearby o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2a785de5e380ad698a24e02aba5d587
https://hdl.handle.net/11391/1535373
https://hdl.handle.net/11391/1535373
Autor:
Kaho Morii, Patricio Sanhueza, Fumitaka Nakamura, James M. Jackson, Shanghuo Li, Henrik Beuther, Qizhou Zhang, Siyi Feng, Daniel Tafoya, Andrés E. Guzmán, Natsuko Izumi, Takeshi Sakai, Xing Lu, Ken’ichi Tatematsu, Satoshi Ohashi, Andrea Silva, Fernando A. Olguin, Yanett Contreras
Publikováno v:
The Astrophysical Journal, 929(1)
This is a correction for 2021 ApJ 923 147DOI 10.3847/1538-4357/ac2365
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d10d7cbf74b62fee6b55cd97f1e1a95a
https://hdl.handle.net/1887/3562734
https://hdl.handle.net/1887/3562734