Figure 6 from THE O- AND B-TYPE STELLAR POPULATION IN W3: BEYOND THE HIGH-DENSITY LAYER

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THE O- AND B-TYPE STELLAR POPULATION IN W3: BEYOND THE HIGH-DENSITY LAYER

Authors: Megan M. Kiminki, Jinyoung Serena Kim, Micaela B. Bagley, William H. Sherry, and George H. Rieke

2015 The Astrophysical Journal 813 42.

Provider: AAS Journals

Caption: Figure 6.

Map of Hα emission across W3 measured from 6083 Hectospec sky spectra (270 lpm). The bright central region is IC 1795; the left edge of the image is part of the W4 H II region. The equivalent widths have an average uncertainty of ±1 Å.

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