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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 7.

Normalized spectra of representative O- and B-type systems in W3. Dotted lines mark the key features used in spectral classification (green: hydrogen; red: He I; blue: He II; black: metals). All spectra in this figure were taken using Hectospec’s 270 lines mm−1 grating.

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