Figure 11 from H II Region Luminosity Function of the Interacting Galaxy M51

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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 11.

Evolution of simulated H ii LFs for four ages (0, 2, 4, and 6 Myr), the parent power-law index β = −2.40, and the maximum number of stars per cluster N _{*, max} = 10,000. Thick solid lines represent power-law fits for L > 10 ^37.0 erg s ⁻¹. The values of the index (α) are given in each panel.

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