Massive Star Formation in the Molecular Ring Orbiting the Black Hole at the Galactic Center

Abstract

A ring of dense molecular gas extending 2-7 pc orbits the supermassive black hole Sgr A* at the center of our Galaxy. Using the Green Bank Telescope, we detected water maser lines and both narrow (0.35 km/s) and broad (30 - 50 km/s) methanol emission from the molecular ring. Two of the strongest methanol lines at 44 GHz are confirmed as masers by interferometric observations. These class I methanol masers are collisionally excited and are signatures of early phases of massive star formation in the disk of the Galaxy, suggesting that star formation in the molecular ring is in its early phase. Close inspection of the kinematics of the associated molecular clumps in the HCN (J=1-0) line reveals broad red-shifted wings indicative of disturbance by protostellar outflows from young (few times 10^4 yr), massive stars embedded in the clumps. The thermal methanol profile has a similar shape, with a narrow maser line superimposed on a broad, red-shifted wing. Additional evidence for the presence of young massive protostars is provided by shocked molecular hydrogen and a number of striking ionized and molecular linear filaments in the vicinity of methanol sources suggestive of 0.5-pc scale protostellar jets. Given that the circumnuclear molecular ring is kinematically unsettled and thus is likely be the result of a recent capture, the presence of both methanol emission and broad, red-shifted HCN emission suggests that star formation in the circumnuclear ring is in its infancy.

13 pages, 4 figures, ApJ Letters (in press)

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• The Excitation of HCN and HCO+ in the Galactic Center Circumnuclear Disk
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• Expanded Very Large Array Detection of 44.1 GHz Class I Methanol Masers in Sagittarius A
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• Mass Distribution in the Central Few Parsecs of Our Galaxy
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• Perturbations induced by a molecular cloud on the young stellar disc in the Galactic Centre
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• A Radio Survey of Galactic Center Clouds
• The Origin of Parsec-Scale Gaseous and Stellar Disks in the Galactic Center and AGNs
• Herschel water maps towards the vicinity of the black hole Sgr A*
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• Molecular gas in the immediate vicinity of Sgr A* seen with ALMA
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