Molecular Gas Feeding the Circumnuclear Disk of the Galactic Center

@article{Hsieh2017MolecularGF,
  title={Molecular Gas Feeding the Circumnuclear Disk of the Galactic Center},
  author={Pei-Ying Hsieh and Patrick M. Koch and Paul T. P. Ho and Woong-Tae Kim and Ya-Wen Tang and Hsiang-Hsu Wang and Hsi-Wei Yen and Chorng-Yuan Hwang},
  journal={The Astrophysical Journal},
  year={2017},
  volume={847}
}
The interaction between a supermassive black hole (SMBH) and the surrounding material is of primary importance in modern astrophysics. The detection of the molecular 2 pc circumnuclear disk (CND) immediately around the Milky Way SMBH, SgrA*, provides a unique opportunity to study SMBH accretion at subparsec scales. Our new wide-field CS(J = 2 − 1) map toward the Galactic center (GC) reveals multiple dense molecular streamers that originated from the ambient clouds 20 pc further out, and that… 

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