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Star Formation in the H I Bridge Between M81 and M82

  • Authors: D. F. de Mello, L. J. Smith, E. Sabbi, J. S. Gallagher, M. Mountain, and D. R. Harbeck

DE MELLO et al. 2008 The Astronomical Journal 135 548.

  • Provider: AAS Journals

Caption: Figure 6.

Color–magnitude diagram, F814W versus F475W − F814W (~ I versus  B − I), of all stars measured in the ACS field of view. Superimposed on the CMD are Padova isochrones (Fagotto et al. 1994a, 1994b), with a metallicity Z = 0.004 and ages 7 Myr to 10 Gyr.

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