Supernovae generated High Velocity Compact Clouds

Abstract

It has been proposed that an intermediate mass black hole can produce compact molecular clouds with large velocity dispersions. This model is called into question due to the discovery of several such short lived clouds, which suggests they are common, and hence it is unlikely that their formation involves an exotic object such as an intermediate mass black hole. In this paper we propose an alternative model, where supernovae produce such clouds. We apply our model to a such a cloud called CO-0.40-0.22. A previous work pointed out the fact that the kinetic energy of this cloud is comparable to that from a supernova, but disqualified the supernova scenario due to lack of thermal emission. We explain the lack of thermal emission as a consequence of the large density of the medium. In such a medium, the supernova shock is radiation dominated, and hence the initial temperatures are lower by many orders of magnitude compared with a typical supernova. Finally, we discuss some of the consequences of having a significant population of intermediate mass black holes in the galactic centre.

References in corpus (6)

• The rate and latency of star formation in dense, massive clumps in the Milky Way
• Signature of an Intermediate-Mass Black Hole in the Central Molecular Zone of Our Galaxy
• Supernova Feedback in Molecular Clouds: Global Evolution and Dynamics
• Millimetre-wave Emission from an Intermediate-Mass Black Hole Candidate in the Milky Way
• Radio polarimetry of Galactic centre pulsars
• Discovery of Two Small High-Velocity Compact Clouds in the Central 10 Parsecs of Our Galaxy

Cited by in corpus (4)

• Intermediate-Mass Black Holes
• Indication of Another Intermediate-mass Black Hole in the Galactic Center
• The Fifth Candidate for an Intermediate-mass Black Hole in the Galactic Center
• An energetic high-velocity compact cloud: CO$-$0.31+0.11