Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-05T03:28:50.824Z Has data issue: false hasContentIssue false
  • English
  • Français

Molecular Line Observations in Sgr B2

Published online by Cambridge University Press:  04 August 2017

Masaki Morimoto ,
Masatoshi Ohishi  and
Tomio Kanzawa
Masaki Morimoto
Affiliation:
Nobeyama Radio Observatory, Japan
Masatoshi Ohishi
Affiliation:
Nobeyama Radio Observatory, Japan
Tomio Kanzawa
Affiliation:
Nobeyama Radio Observatory, 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.

The ∼20 pc square region around the continuum peak, (α(1950.0) = 17h44m 10.6s, δ(1950.0) = −28°22′05″) of Sgr B2 was observed using the 45-m telescope of Nobeyama Radio Observatory. The observed molecules are H2O, NH3, CH3OH, SiO, H13CN, H13CO+, CO, HNCO, HC3N, and so on.

Type
I. Star Forming Processes in the Solar Neighborhood
Information
Symposium - International Astronomical Union , Volume 115: Star Forming Regions , 1987 , pp. 156 - 158
Copyright
Copyright © Reidel 1987