Maser Emission toward the Infrared Dark Cloud G359.94+0.17 Seen in Silhouette against the Galactic Center
arXiv:1109.0677 · doi:10.1093/pasj/64.2.28
Abstract
The infrared dark cloud G359.94+0.17 is a conspicuous, opaque cloud, which is seen in silhouette against the Galactic center. We found unexpectedly strong (~50 Jy) maser emission of CH3OH at 44 GHz with additional weak 22 GHz H2O maser and 43 GHz SiO thermal emissions toward this cloud. Detections of these molecular lines indicate that strong star forming activities are proceeding in this cloud, which were not reported previously despite of numerous works toward the Galactic center. The line profiles of the NH3 inversion lines at 23 GHz indicate that G359.94+0.17 is composed of mainly two clouds with V(lsr)= 0, and 15 km/s overlapped on the line of sight. The maser emission is associated with the 15 km/s cloud, suggesting that it is located at the Norma spiral arm.
PASJ 64, no2 (April 25, 2012 issue) in press
References in corpus (7)
- A 100-parsec elliptical and twisted ring of cold and dense molecular clouds revealed by Herschel around the Galactic Center
- A Class I and Class II Methanol Maser Survey of Extended Green Objects (EGOs) from the GLIMPSE Survey
- Star Formation in the Central 400 pc of the Milky Way: Evidence for a Population of Massive YSOs
- A statistical study of the mass and density structure of Infrared Dark Clouds
- A Multi-Epoch, Simultaneous Water and Methanol Maser Survey toward Intermediate-Mass Young Stellar Objects
- Methanol Maser Emission from Galactic Center Sources with Excess 4.5 μm Emission
- The ASTE Galactic Center CO J=3-2 Survey: Probing Shocked Molecular Gas in the CMZ