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Variation in GMC Association Properties across the Bars, Spiral Arms, Inter-arms, and Circumnuclear Region of M100 (NGC 4321) Extracted from ALMA Observations

  • Authors: Hsi-An Pan and Nario Kuno

2017 The Astrophysical Journal 839 133.

  • Provider: AAS Journals

Caption: Figure 2.

Representative spectral lines at the galactic center (gc), CNR, bar, spiral, and inter-arm regions. The noise level in the spectral data cube is ∼0.015 Jy beam−1.

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