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Unveiling the Nature of M94's (NGC4736) Outer Region: A Panchromatic Perspective

  • Authors: Ignacio Trujillo, Inma Martinez-Valpuesta, David Martínez-Delgado, Jorge Peñarrubia, R. Jay Gabany, and Michael Pohlen

TRUJILLO et al. 2009 The Astrophysical Journal 704 618.

  • Provider: AAS Journals

Caption: Figure 9.

Left panel: snapshot of the SPH simulation showing the spiral arms as a response to the inner oval distortion. Right panel: the solid line shows the gas surface density profile of our model. The different peaks represent the response of the gas to the dynamical effect of the oval distortion. The dashed line shows the FUV surface brightness (i.e., a good proxy to the recent star formation) scaled to fit in the plot.

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