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H II Region Luminosity Function of the Interacting Galaxy M51

  • Authors: Jong Hwan Lee, Narae Hwang, and Myung Gyoon Lee

Lee, Hwang, & Lee 2011 The Astrophysical Journal 735 75.

  • Provider: AAS Journals

Caption: Figure 7.

Size distribution of the H ii regions in the original sample. (a) Cumulative size distribution. The solid line represents an exponential fit. (b) Differential size distribution. Thick dashed and thick solid lines represent a double power-law fit with a break at log D = 1.45 ( D ≈ 30 pc). The power-law index for small H ii regions with D < 30 pc is α D = −5.04 ± 0.08, whereas α D = −1.78 ± 0.04 for large H ii regions with D > 30 pc. An arrow marks the break point.

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