Zobrazeno 1 - 10
of 46
pro vyhledávání: '"NISHIURA,Shingo"'
We have studied optical properties of interstellar dust around the Orion A molecular cloud to investigate the size distribution and the composition of dust grains. Orion A is one of the most studied molecular clouds in the solar vicinity ($d \simeq 4
Externí odkaz:
http://arxiv.org/abs/2107.01043
Autor:
Nakajima, Taku, Kaiden, Masahiro, Korogi, Jun, Kimura, Kimihiro, Yonekura, Yoshinori, Ogawa, Hideo, Nishiura, Shingo, Dobashi, Kazuhito, Handa, Toshihiro, Kohno, Kotaro, Morino, Jun-Ichi, Asayama, Shin'ichiro, Noguchi, Takashi
We have upgraded the 60-cm radio survey telescope located in Nobeyama, Japan. We developed a new waveguide-type sideband-separating SIS mixer for the telescope, which enables the simultaneous detection of distinct molecular emission lines both in the
Externí odkaz:
http://arxiv.org/abs/0706.1353
Autor:
Shioya, Yasuhiro, Taniguchi, Yoshiaki, Murayama, Takashi, Nishiura, Shingo, Nagao, Tohru, Kakazu, Yuko
Publikováno v:
Astrophys.J. 576 (2002) 36-44
First-generation (Population III) stars in the universe play an important role inearly enrichment of heavy elements in galaxies and intergalactic medium and thus affect the history of galaxies. The physical and chemical properties of primordial gas c
Externí odkaz:
http://arxiv.org/abs/astro-ph/0205153
Autor:
Taniguchi, Yoshiaki, Ohyama, Youichi, Murayama, Takashi, Yoshida, Michitoshi, Kashikawa, Nobunari, Iye, Masanori, Aoki, Kentaro, Sasaki, Toshiyuki, Kosugi, George, Takata, Tadafumi, Saito, Yoshihiko, Kawabata, Koji S., Sekiguchi, Kazuhiro, Okita, Kiichi, Shimizu, Yasuhiro, Inata, Motoko, Ebizuka, Noboru, Ozawa, Tomohiko, Yadomaru, Yasushi, Taguchi, Hiroko, Shioya, Yasuhiro, Nishiura, Shingo, Sudou, Hiroshi, Nagao, Tohru, Noda, Saeko, Kakazu, Yuko, Ajiki, Masaru, Fujita, Shinobu S., Kobayashi, Rie R.
We present new optical spectroscopy of the high-redshift powerful radio galaxy MRC 0406$-$244 at redshift of 2.429. We find that the two extensions toward NW and SE probed in the rest-frame ultraviolet image are heated mainly by the nonthermal contin
Externí odkaz:
http://arxiv.org/abs/astro-ph/0108126
In order to investigate the nuclear activity of galaxies residing in compact groups of galaxies, we present results of our optical spectroscopic program made at Okayama Astrophysical Observatory. We have performed optical spectroscopy of 69 galaxies
Externí odkaz:
http://arxiv.org/abs/astro-ph/0003056
Autor:
Murayama, Takashi, Nishiura, Shingo, Nagao, Tohru, Sato, Yasunori, Taniguchi, Yoshiaki, Sanders, D. B.
Publikováno v:
Astron.J. 119 (2000) 1691-1694
We report the discovery of a low surface brightness (LSB) object serendipitously found during deep CCD imaging of a compact group of galaxies, Seyfert's Sextet, in VR and I bands. The LSB object is located 2.3 arcmin southwest from the group center.
Externí odkaz:
http://arxiv.org/abs/astro-ph/0001071
The origin of huge infrared luminosities of ultraluminous infrared galaxies (ULIGs) is still in question. Recently, Genzel et al. made mid-infrared (MIR) spectroscopy of a large number of ULIGs and found that the major energy source in them is massiv
Externí odkaz:
http://arxiv.org/abs/astro-ph/9810249
Autor:
ISHII,Natsumi, NISHIURA,Shingo, ITOH,Nobunari, YAMAGATA,Tomohiko, HAMABE,Masaru, SHIMOIKURA,Tomomi
Publikováno v:
東京学芸大学紀要. 自然科学系. 72:53-65
Publikováno v:
東京学芸大学紀要. 自然科学系. 70:73-85
Publikováno v:
東京学芸大学紀要. 自然科学系. 69:129-135