Star-forming Cloud Complexes in the Central Molecular Zone of NGC 253

@article{Sakamoto2011StarformingCC,
  title={Star-forming Cloud Complexes in the Central Molecular Zone of NGC 253},
  author={Kazushi Sakamoto and Ruiqing Mao and Satoki Matsushita and Alison B. Peck and Tsuyoshi Sawada and Martina C. Wiedner},
  journal={The Astrophysical Journal},
  year={2011},
  volume={735},
  pages={19}
}
We report 350 and 230 GHz observations of molecular gas and dust in the starburst nucleus of NGC 253 at 20-40 pc (1 ''-2 '') resolution. The data contain CO(3-2), HCN(4-3), CO(2-1), (CO)-C-13(2-1), (CO)-O-18(2-1), and continuum at 0.87 mm and 1.3 mm toward the central kiloparsec. The CO(2-1) size of the galaxy's central molecular zone (CMZ) is measured to be about 300 pc x 100 pc at the half-maximum of intensity. Five clumps of dense and warm gas stand out in the CMZ at arcsecond resolution… Expand

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