Zobrazeno 1 - 10
of 246
pro vyhledávání: '"Matsumura, Shinji"'
Autor:
Nishida, Kazuhiko1 (AUTHOR) nishidka@hirakata.kmu.ac.jp, Matsumura, Shinji1 (AUTHOR), Uchida, Hitoshi2 (AUTHOR), Abe, Manabu2,3 (AUTHOR), Sakimura, Kenji2,3 (AUTHOR), Badea, Tudor Constantin4,5 (AUTHOR), Kobayashi, Takuya1 (AUTHOR)
Publikováno v:
PLoS ONE. 9/21/2023, Vol. 18 Issue 9, p1-28. 28p.
Publikováno v:
Home Health Care Management & Practice; Nov2024, Vol. 36 Issue 4, p262-279, 18p
Autor:
Matsumura, Shinji1 (AUTHOR) matsusnj@bosai.go.jp, Horinouchi, Takeshi2 (AUTHOR)
Publikováno v:
Journal of Climate. Apr2023, Vol. 36 Issue 8, p2483-2496. 14p.
Autor:
Takekawa, Shunya, Oka, Tomoharu, Tanaka, Kunihiko, Matsumura, Shinji, Miura, Kodai, Sakai, Daisuke
We have performed unbiased spectral line surveys at 3 mm band toward the Galactic circumnuclear disk (CND) and Sgr A* using the Nobeyama Radio Observatory (NRO) 45 m radio telescope. The target positions are two tangential points of the CND and the d
Externí odkaz:
http://arxiv.org/abs/1407.4880
Autor:
Sakai, Daisuke, Oka, Tomoharu, Tanaka, Kunihiko, Matsumura, Shinji, Miura, Kodai, Takekawa, Shunya
We report the results of millimeter-wave molecular line observations of the Tornado Nebula (G357.7--0.1), which is a bright radio source behind the Galactic Center region. A 15'x15' area was mapped in the J=1--0 lines of CO, 13CO, and HCO+ with the N
Externí odkaz:
http://arxiv.org/abs/1407.3273
Akademický článek
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We report the detection of extremely broad emission toward two molecular clumps in the Galactic central molecular zone. We have mapped the Sagittarius C complex ($-0^\circ.61 < l < -0^\circ.27$, $-0^\circ.29 < b < 0^\circ.04$) in the HCN $J$ = 4--3,
Externí odkaz:
http://arxiv.org/abs/1402.1335
Publikováno v:
Journal of Climate, 2019 Apr . 32(8), 2247-2259.
Externí odkaz:
https://www.jstor.org/stable/26662912
Autor:
Sashida, Tomoro, Oka, Tomoharu, Tanaka, Kunihiko, Aono, Kazuya, Matsumura, Shinji, Nagai, Makoto, Seta, Masumichi
We mapped molecular gas toward the supernova remnant W44 in the HCO+ J=1-0 line with the Nobeyama Radio Observatory 45 m telescope and in the CO J=3-2 line with the Atacama Submillimeter Telescope Experiment 10 m telescope. High-velocity emission win
Externí odkaz:
http://arxiv.org/abs/1307.6276
Autor:
Matsumura, Shinji, Oka, Tomoharu, Tanaka, Kunihiko, Nagai, Makoto, Kamegai, Kazuhisa, Hasegawa, Tetsuo
This paper reports the discovery of a helical molecular cloud in the central molecular zone (CMZ) of our Galaxy. This "pigtail" molecular cloud appears at (l, b, V_LSR) ~ (-0.7deg, +0.0deg, -70 to -30 km/s), with a spatial size of ~ (20 pc)^2 and a m
Externí odkaz:
http://arxiv.org/abs/1207.4704