Hostname: page-component-78c5997874-xbtfd Total loading time: 0 Render date: 2024-11-19T07:32:08.512Z Has data issue: false hasContentIssue false
  • English
  • Français

4.4. The Sagittarius C region mapped in CS(2→1) and (3→2) by the IRAM 30m telescope

Published online by Cambridge University Press:  25 May 2016

C. Kramer ,
J. Staguhn ,
H. Ungerechts  and
A. Sievers
C. Kramer
Affiliation:
I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany
J. Staguhn
Affiliation:
University of Maryland, Department of Astronomy, College Park, MD 20742-2421, USA
H. Ungerechts
Affiliation:
Instituto de Radioastronomia Milimetrica, Avenida Divina Pastora 7, 18012 Granada, Spain
A. Sievers
Affiliation:
Instituto de Radioastronomia Milimetrica, Avenida Divina Pastora 7, 18012 Granada, Spain

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.

We study the interaction of a dense giant molecular cloud with the HII region Sagittarius C, and a prominent nonthermal filament (NTF). For this purpose, we mapped the CS(2→1) and (3→2) transitions simultaneously with the IRAM 30m radio telescope, using the on-the-fly observing mode, and covering a 20pc×37pc (8′ × 15′) region. The high spatial resolution, 0.7pc (16″) at 147 GHz, allows for the first time to analyze in detail the morphology and kinematics of the molecular material and its relation to the ionized gas.

Type
Part II. Nuclear Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 173 - 174
Copyright
Copyright © Kluwer 1998 

References

Liszt, H.S., Spiker, R.W., 1995, ApJS, 98, 259 (LS95).Google Scholar