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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 3.

H ii LF for the original sample (histogram). Thick dashed and thick solid lines represent a double power-law fit for the faint part ( L < 10 37.1 erg s −1) and the bright part ( L > 10 37.1 erg s −1), respectively. The power-law indices are α = −2.25 ± 0.02 for the bright part and α = −1.42 ± 0.01 for the faint part. An arrow marks the break point.

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