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Star Formation Histories of the LEGUS Spiral Galaxies. I. The Flocculent Spiral NGC 7793

  • Authors: E. Sacchi, M. Cignoni, A. Aloisi, M. Tosi, A. Adamo, D. A. Dale, B. G. Elmegreen, D. M. Elmegreen, D. Calzetti, D. A. Gouliermis, K. Grasha, L. J. Smith, A. Wofford, J. C. Lee, E. Sabbi, and L. Ubeda

2019 The Astrophysical Journal 878 1.

  • Provider: AAS Journals

Caption: Figure 13.

Optical SFR surface densities (SFR/area; left panel) and cumulative stellar mass fraction (right panel) as a function of time in different regions of NGC 7793, from the COLIBRI solutions. The right-hand plot also shows a comparison with a constant SFH (black solid line) and a reference for an age of 1 Gyr (vertical dotted line) and for 50% of the total assembled mass (horizontal dotted line).

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