Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-29T13:30:25.821Z Has data issue: false hasContentIssue false
  • English
  • Français

Aperture Synthesis Obervations of The Galactic Center 50-km·s−1 Moleculer Could

Published online by Cambridge University Press:  12 April 2016

Masato Tsuboi ,
Sachiko K. Okumura  and
Masato Ishiguro
Masato Tsuboi
Affiliation:
Nobeyama Radio Observatory, Minamisaku, Nagano, 384-13, Japan
Sachiko K. Okumura
Affiliation:
Nobeyama Radio Observatory, Minamisaku, Nagano, 384-13, Japan
Masato Ishiguro
Affiliation:
Nobeyama Radio Observatory, Minamisaku, Nagano, 384-13, Japan

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Molecular clouds in the Galactic center region are distributed mainly along the Galactic plane and have filamentary shapes with several clumps (Bally et al. 1987, Tsuboi et al. 1989). The “50-km.s−1 molecular cloud (M-0.02-0.07)”, which is located ~3’ east from Sgr A West, is one of most remarkable clumps on these molecular filaments. The intimate relation between this cloud and Sgr A East has been mentioned by many authers (e.g. Ho et al. 1986). Several compact HII regions are located toward the cloud (Ekers et al. 1983). The recombination line velocities correspond to the molecular line velocities in the cloud (Goss et al. 1987). Thus this cloud is one of active star forming regions near the Galactic center.

We observed the 50-km-s−1 molecular cloud in CS J=1-0 emission line (48.991 GHz) using the Nobeyama Millimeter Array (NMA) to reveal the detailed structure of the star forming regions near the Galactic center.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 170 - 171
Copyright
Copyright © Astronomical Society of the Pacific 1994

References

Bally, J. et al., 1987, Astrophys. J. Suppl., 65, 13.Google Scholar
Ekers, R.D. et al., 1983, Astron. Astrophys., 122, 143.Google Scholar
Goss, W.M. et al., 1987, MNRAS, 215, 69p.Google Scholar
Ho, P.T.P. et al., 1985, Astophys. J., 288, 575.Google Scholar
Tsuboi, M. et al., 1989, Proc. of the IAU Symposium No. 136, 135.Google Scholar
Yusef-Zadeh, F. and Morris, M., 1987a, Astophys. J., 320, 545.Google Scholar
Yusef-Zadeh, F. and Morris, M., 1987b, Astophys. J., 322, 721.Google Scholar