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of 433
pro vyhledávání: '"Miyazaki, Atsushi"'
Autor:
Petry, Dirk, Trigo, María Díaz, Kneissl, Rüdiger, Toledo, Ignacio, Miyazaki, Atsushi, Takagi, Toshinobu, Barnes, Ashley, Bonanomi, Francesca
The Atacama Large Millimeter/submillimeter Array remains the largest mm radio interferometer observatory world-wide. It is now conducting its 11th observing cycle. In our previous paper presented at this conference series in 2020, we outlined a numbe
Externí odkaz:
http://arxiv.org/abs/2406.13199
Atacama Large Millimeter/Submillimeter Array (ALMA) is promising to be a powerful tool for precision astrometry of the area around Sagittarius A$^\ast$ (Sgr A$^\ast$) because it has the high angular resolution, high sensitivity, and wide field of vie
Externí odkaz:
http://arxiv.org/abs/2204.06778
We present the results based on the 2.5 arcsec-resolution observations using Atacama Large Millimeter/submillimeter Array (ALMA) of the Galactic Center Molecular Cloud G-0.02-0.07, or the 50 km/s Molecular Cloud (50MC), in the SO (N_J=2_2-1_1) line a
Externí odkaz:
http://arxiv.org/abs/2105.09449
Autor:
Inoue, Shigeki, Takagi, Toshinobu, Miyazaki, Atsushi, Cooper, Erin Mentuch, Egusa, Fumi, Yajima, Hidenobu
We investigate dynamical states of grand-design spiral arms in three local galaxies: M51, NGC3627 and NGC628. Based on linear perturbation analysis considering multiple components in the galaxies, we compute instability parameters of the spiral arms
Externí odkaz:
http://arxiv.org/abs/2103.12130
Publikováno v:
BMC Anesthesiology. 4/22/2024, Vol. 24 Issue 1, p1-8. 8p.
Autor:
Tsuboi, Masato, Kitamura, Yoshimi, Uehara, Kenta, Miyawaki, Ryosuke, Tsutsumi, Takahiro, Miyazaki, Atsushi, Miyoshi, Makoto
We performed a search of cloud-cloud collision (CCC) sites in the Sagittarius A molecular cloud (SgrAMC) based on the survey observations using the Nobeyama 45-m telescope in the C$^{32}$S $J=1-0$ and SiO $v=0~J=2-1$ emission lines. We found candidat
Externí odkaz:
http://arxiv.org/abs/2009.11461
Autor:
Tsuboi, Masato, Tsutsumi, Takahiro, Kitamura, Yoshimi, Miyawaki, Ryosuke, Miyazaki, Atsushi, Miyoshi, Makoto
The Galactic Center Lobe (GCL) is a peculiar object widely protruding from the Galactic plane toward the positive Galactic latitude, which had been found toward the Galactic Center (GC) in the early days of the radio observation. The peculiar shape h
Externí odkaz:
http://arxiv.org/abs/2007.09673
Autor:
Tsuboi, Masato, Kitamura, Yoshimi, Tsutsumi, Takahiro, Miyawaki, Ryosuke, Miyoshi, Makoto, Miyazaki, Atsushi
The Galactic Center IRS 13E cluster is a very intriguing IR object located at $\sim0.13$ pc from Sagittarius A$^\ast$ (Sgr A$^\ast$) in projection distance. There are both arguments for and against the hypothesis that a dark mass like an intermediate
Externí odkaz:
http://arxiv.org/abs/2002.08508
Autor:
Tsuboi, Masato, Kitamura, Yoshimi, Tsutsumi, Takahiro, Miyawaki, Ryosuke, Miyoshi, Makoto, Miyazaki, Atsushi
IRS 7 is an M red supergiant star which is located at $5".5$ north of Sagittarius A$^\ast$. We detected firstly the continuum emission at 340 GHz of IRS 7 using ALMA. The total flux density of IRS 7 is $S_\nu=448\pm45 \mu$Jy. The flux density indicat
Externí odkaz:
http://arxiv.org/abs/2002.01620
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