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Models of the Morphology, Kinematics, and Star Formation History of the Prototypical Collisional Starburst System NGC 7714/7715 = ARP 284

  • Authors: Curtis Struck and Beverly J. Smith

Struck & Smith 2003 The Astrophysical Journal 589 157.

  • Provider: AAS Journals

Caption: Fig. 19.

Velocity of model gas particles in the z‐direction vs. x‐coordinate value for comparison with observational velocity–right ascension plot. Note that we have rotated the model results by −10° in the xy plane, so that the x‐axis of the model more nearly corresponds to right ascension. The model velocities have been scaled as in Fig. 18, multiplying by a factor of 100 and adding a constant systemic velocity of 2800 km s−1. The x‐axis values are in dimensionless code units. Text labels identify particle sets corresponding to those of the observational plot (Fig. 20). See text for details.

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