We present high-resolution (~2-3"; ~0.1 pc) radio observations of the Galactic center cloud M0.10-0.08 using the Very Large Array at K and Ka band (~25 and 36 GHz). The M0.10-0.08 cloud is located in a complex environment near the Galactic center Radio Arc and the adjacent M0.11-0.11 molecular cloud. From our data, M0.10-0.08 appears to be a compact molecular cloud (~3 pc) that contains multiple compact molecular cores (5+; <0.4 pc). In this study we detect a total of 15 molecular transitions in M0.10-0.08 from the following molecules: NH3, HC3N, CH3OH, HC5N, CH3CN, and OCS. We have identified more than sixty 36 GHz CH3OH masers in M0.10-0.08 with brightness temperatures above 400 K and 31 maser candidates with temperatures between 100-400 ...
New HI images from the VLA Galactic Plane Survey (VGPS) show clear absorption features associated wi...
Recent observations indicate that the cosmic rate ionization rate in the Galactic center is higher t...
We present a synthesis of a number of recent observations in the near-IR H_2 and [Fe II] lines, OH (...
Context. The 1°.3 (G1.3) and 1°.6 (G1.6) cloud complexes in the central molecular zone (CMZ) of our ...
We have analysed the chemical and kinematic properties of the 20 and 50 km s−1 molecular clouds in t...
A model is proposed in which most of the molecular clouds near the galactic center are situated in a...
Interstellar molecular clouds play an essential role in the Universe. Such clouds are invoked for th...
We used the Atacama Pathfinder Experiment (APEX) 12 m telescope to observe the J(KAKc) = 3(03) -> 2(...
Observations of the 2.6-mm CO line have been obtained along the galactic equator covering longitudes...
Molecular gas temperatures in the Galactic Center have been shown to much higher than the gas temper...
We universally search for evidence of kinematic and spatial correlation of supernova remnant (SNR) a...
In the centres of the Milky Way and M83, the global environmental properties thought to control star...
3C 397 is a radio and X-ray bright Galactic supernova remnant (SNR) with an unusual rectangular morp...
We present dense-gas--tracing molecular observations of six resolved Giant Molecular Clouds (GMCs) i...
We present new, high-angular resolution interferometric observations with the Karl G. Jansky Very La...
New HI images from the VLA Galactic Plane Survey (VGPS) show clear absorption features associated wi...
Recent observations indicate that the cosmic rate ionization rate in the Galactic center is higher t...
We present a synthesis of a number of recent observations in the near-IR H_2 and [Fe II] lines, OH (...
Context. The 1°.3 (G1.3) and 1°.6 (G1.6) cloud complexes in the central molecular zone (CMZ) of our ...
We have analysed the chemical and kinematic properties of the 20 and 50 km s−1 molecular clouds in t...
A model is proposed in which most of the molecular clouds near the galactic center are situated in a...
Interstellar molecular clouds play an essential role in the Universe. Such clouds are invoked for th...
We used the Atacama Pathfinder Experiment (APEX) 12 m telescope to observe the J(KAKc) = 3(03) -> 2(...
Observations of the 2.6-mm CO line have been obtained along the galactic equator covering longitudes...
Molecular gas temperatures in the Galactic Center have been shown to much higher than the gas temper...
We universally search for evidence of kinematic and spatial correlation of supernova remnant (SNR) a...
In the centres of the Milky Way and M83, the global environmental properties thought to control star...
3C 397 is a radio and X-ray bright Galactic supernova remnant (SNR) with an unusual rectangular morp...
We present dense-gas--tracing molecular observations of six resolved Giant Molecular Clouds (GMCs) i...
We present new, high-angular resolution interferometric observations with the Karl G. Jansky Very La...
New HI images from the VLA Galactic Plane Survey (VGPS) show clear absorption features associated wi...
Recent observations indicate that the cosmic rate ionization rate in the Galactic center is higher t...
We present a synthesis of a number of recent observations in the near-IR H_2 and [Fe II] lines, OH (...