Zobrazeno 1 - 10
of 1 918
pro vyhledávání: '"Saigo, P"'
Autor:
Tachihara, Kengo, Fukaya, Naofumi, Tokuda, Kazuki, Yamasaki, Yasumasa, Nishioka, Takeru, Abe, Daisei, Inoue, Tsuyoshi, Harada, Naoto, Shoshi, Ayumu, Nozaki, Shingo, Sato, Asako, Omura, Mitsuki, Fujishiro, Kakeru, Fukagawa, Misato, Machida, Masahiro N., Kanai, Takahiro, Oasa, Yumiko, Onishi, Toshikazu, Saigo, Kazuya, Fukui, Yasuo
We report on ALMA ACA observations of a high-density region of the Corona Australis cloud forming a young star cluster, and the results of resolving internal structures. In addition to embedded Class 0/I protostars in continuum, a number of complex d
Externí odkaz:
http://arxiv.org/abs/2404.11113
Autor:
Tokuda, Kazuki, Harada, Naoto, Omura, Mitsuki, Matsumoto, Tomoaki, Onishi, Toshikazu, Saigo, Kazuya, Shoshi, Ayumu, Nozaki, Shingo, Tachihara, Kengo, Fukaya, Naofumi, Fukui, Yasuo, Inutsuka, Shu-ichiro, Machida, Masahiro N.
Recent Atacama Large Millimeter/submillimeter Array (ALMA) observations have revealed an increasing number of compact protostellar disks with radii of less than a few tens of astronomical units and that young Class 0/I objects have an intrinsic size
Externí odkaz:
http://arxiv.org/abs/2403.00305
Autor:
Takahashi, Satoko, Machida, Masahiro N., Omura, Mitsuki, Johnstone, Doug, Saigo, Kazuya, Harada, Naoto, Tomisaka, Kohji, Ho, Paul T. P., Zapata, Luis A., Mairs, Steve, Herczeg, Gregory J., Taniguchi, Kotomi, Liu, Yuhua, Sato, Asako
We present ${\sim}0.2$ arcsec ($\sim$80 au) resolution observations of the CO (2-1) and SiO (5-4) lines made with the Atacama large millimeter/submillimeter array toward an extremely young intermediate-mass protostellar source (t$_{\rm dyn}<$1000 yea
Externí odkaz:
http://arxiv.org/abs/2401.13204
Publikováno v:
Res. Math. Sci.,11, article number 62, (2024)
We extend a certain type of identities on sums of $I$-Bessel functions on lattices, previously given by G. Chinta, J. Jorgenson, A. Karlsson and M. Neuhauser. Moreover we prove that, with continuum limit, the transformation formulas of theta function
Externí odkaz:
http://arxiv.org/abs/2311.06489
Autor:
Daichi Kodama, Motoki Takenaka, Chiemi Saigo, Masako Azuma, Yuki Hanamatsu, Masanori Isobe, Tamotsu Takeuchi
Publikováno v:
Journal of Ovarian Research, Vol 17, Iss 1, Pp 1-9 (2024)
Abstract Recent studies have revealed that the Sry-related HMG box gene 17 (SOX17) plays an important role in ovarian carcinogenesis. Unlike other types of ovarian cancer, ovarian clear cell carcinoma (OCCC) has a distinct pathobiological phenotype,
Externí odkaz:
https://doaj.org/article/4ec6e70f56cb410595753ad7e2517d24
Publikováno v:
Thoracic Cancer, Vol 15, Iss 32, Pp 2319-2326 (2024)
Abstract Introduction Sex‐determining region Y‐related high‐mobility group box 17 protein (SOX17), a proangiogenic transcription factor, is specifically expressed in tumor endothelial cells (TECs) of implanted Lewis lung carcinoma. However, the
Externí odkaz:
https://doaj.org/article/3efb8e5db128490e9b742b9cdf31de27
Autor:
Aso, Yusuke, Kwon, Woojin, Ohashi, Nagayoshi, Jorgensen, Jes K., Tobin, John J., Aikawa, Yuri, de Gregorio-Monsalvo, Itziar, Han, Ilseung, Kido, Miyu, Koch, Patrick M., Lai, Shih-Ping, Lee, Chang Won, Lee, Jeong-Eun, Li, Zhi-Yun, Lin, Zhe-Yu Daniel, Looney, Leslie W., Narayanan, Suchitra, Phuong, Nguyen Thi, Sai, Jinshi, Saigo, Kazuya, Santamaria-Miranda, Alejandro, Sharma, Rajeeb, Takakuwa, Shigehisa, Thieme, Travis J., Tomida, Kengo, Williams, Jonathan P., Yen, Hsi-Wei
Publikováno v:
ApJ 954 (2023) 101-117
Precise estimates of protostellar masses are crucial to characterize the formation of stars of low masses down to brown-dwarfs (BDs; M* < 0.08 Msun). The most accurate estimation of protostellar mass uses the Keplerian rotation in the circumstellar d
Externí odkaz:
http://arxiv.org/abs/2309.01891
Autor:
Sai, Jinshi, Yen, Hsi-Wei, Ohashi, Nagayoshi, Tobin, John J., Jørgensen, Jes K., Takakuwa, Shigehisa, Saigo, Kazuya, Aso, Yusuke, Lin, Zhe-Yu Daniel, Koch, Patrick M., Aikawa, Yuri, Flores, Christian, de Gregorio-Monsalvo, Itziar, Han, Ilseung, Kido, Miyu, Kwon, Woojin, Lai, Shih-Ping, Lee, Chang Won, Lee, Jeong-Eun, Li, Zhi-Yun, Looney, Leslie W., Mori, Shoji, Phuong, Nguyen Thi, Santamaría-Miranda, Alejandro, Sharma, Rajeeb, Thieme, Travis J., Tomida, Kengo, Williams, Jonathan P.
We have observed the Class 0/I protostellar system Ced110 IRS4 at an angular resolution of $0.05''$ ($\sim$10 au) as a part of the ALMA large program; Early Planet Formation in the Embedded Disks (eDisk). The 1.3 mm dust continuum emission reveals th
Externí odkaz:
http://arxiv.org/abs/2307.08952
Autor:
Muraoka, Kazuyuki, Konishi, Ayu, Tokuda, Kazuki, Kondo, Hiroshi, Miura, Rie E., Tosaki, Tomoka, Onodera, Sachiko, Kuno, Nario, Kobayashi, Masato I. N., Tsuge, Kisetsu, Sano, Hidetoshi, Kitano, Naoya, Fujita, Shinji, Nishimura, Atsushi, Onishi, Toshikazu, Saigo, Kazuya, Yamada, Rin I., Demachi, Fumika, Tachihara, Kengo, Fukui, Yasuo, Kawamura, Akiko
We present the results of ALMA-ACA 7 m-array observations in $^{12}$CO($J=2-1$), $^{13}$CO($J=2-1$), and C$^{18}$O($J=2-1$) line emission toward the molecular-gas disk in the Local Group spiral galaxy M33 at an angular resolution of 7".31 $\times$ 6"
Externí odkaz:
http://arxiv.org/abs/2307.02039
Autor:
Kido, Miyu, Takakuwa, Shigehisa, Saigo, Kazuya, Ohashi, Nagayoshi, Tobin, John J., K, Jes, Jørgensen, Aikawa, Yuri, Aso, Yusuke, Encalada, Frankie J., Flores, Christian, Gavino, Sacha, de Gregorio-Monsalvo, Itziar, Han, Ilseung, Hirano, Shingo, Koch, Patrick M., Kwon, Woojin, Lai, Shih-Ping, Lee, Chang Won, Lee, Jeong-Eun, Li, Zhi-Yun, Lin, Zhe-Yu Daniel, Looney, Leslie W., Mori, Shoji, Narayanan, Suchitra, Plunkett, Adele L., Phuong, Nguyen Thi, Sai, Jinshi, Santamarîa-Miranda, Alejandro, Sharma, Rajeeb, Sheehan, Patrick, Thieme, Travis J., Tomida, Kengo, Hoff, Merel L. R. van't, Williams, Jonathan P., Yamato, Yoshihide, Yen, Hsi-Wei
We present observations of the Class 0 protostar IRAS 16544-1604 in CB 68 from the ''Early Planet Formation in Embedded Disks (eDisk)'' ALMA Large program. The ALMA observations target continuum and lines at 1.3-mm with an angular resolution of $\sim
Externí odkaz:
http://arxiv.org/abs/2306.15443