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Spatially Resolved Ultraviolet, Hα, Infrared, and Radio Star Formation in M81

  • Authors: K. D. Gordon, P. G. Pérez-González, K. A. Misselt, E. J. Murphy, G. J. Bendo, F. Walter, M. D. Thornley, R. C. Kennicutt, Jr., G. H. Rieke, C. W. Engelbracht, J.-D. T. Smith, A. Alonso-Herrero, P. N. Appleton, D. Calzetti, D. A. Dale, B. T. Draine, D. T. Frayer, G. Helou, J. L. Hinz, D. C. Hines, D. M. Kelly, J. E. Morrison, J. Muzerolle, M. W. Regan, J. A. Stansberry, S. R. Stolovy, L. J. Storrie-Lombardi, K. Y. L. Su, and E. T. Young

Gordon et al. 2004 The Astrophysical Journal Supplement Series 154 215.

  • Provider: AAS Journals

Caption: Fig. 4.

Luminosities for UV and Hα, ratiod to the IR luminosity, plotted vs. the IR luminosity. The IR luminosity is normalized to the area in kpc2 of each extraction aperture. The corresponding SFRs and SFR ratios are indicated on the opposite axes. Representative uncertainties are shown.

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