Distribution of SI II in the Galactic Center
Abstract
A map of the Galactic center region in the forbidden Si II 34.8-micron line is presented. The line emission arises from within the photodissociation region (PDR) associated with the neutral gas ring surrounding an ionized gas core confined within 2 pc of the Galactic center. Si II is a useful probe of the inner regions of the ring since it is always optically thin. The Si II data, when analyzed in conjunction with O I, C II, and molecular measurements, outlines the transition region between the PDR and the surrounding molecular cloud. The Si II emission is found to extend beyond that of the O II into the neutral gas ring. Although the interpretation is not unique, the data are consistent with a constant gas-phase abundance of silicon within the inner part of the PDR while the gaseous silicon is depleted by molecule formation in the transition region.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- July 1988
- DOI:
- 10.1086/166513
- Bibcode:
- 1988ApJ...330..803G
- Keywords:
-
- Abundance;
- Galactic Nuclei;
- Line Spectra;
- Milky Way Galaxy;
- Molecular Clouds;
- Silicon;
- Carbon;
- Forbidden Transitions;
- Ionized Gases;
- Neutral Gases;
- Optical Thickness;
- Oxygen;
- Photodissociation;
- Astrophysics;
- GALAXIES: THE GALAXY;
- GALAXIES: NUCLEI;
- INTERSTELLAR: ABUNDANCES;
- INTERSTELLAR: MOLECULES;
- RADIATION MECHANISMS