Fig. 2 from Spatially Resolved Ultraviolet, Hα, Infrared, and Radio Star Formation in M81

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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. 2.

MIPS and ancillary images of M81 shown convolved to have the 160 μm PSF that introduces a prominent Airy ring around bright point sources. The field of view of the images is ﹩15^{\prime }\times 23^{\prime }﹩. Bright foreground stars were masked in the UV and Hα images prior to convolution. The ellipse denotes the region discussed in § 3.1.

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