Figure 11 from MUSE Observations of NGC330 in the Small Magellanic Cloud: Helium Abundance of Bright Main-sequence Stars

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MUSE Observations of NGC330 in the Small Magellanic Cloud: Helium Abundance of Bright Main-sequence Stars

Authors: R. Carini, K. Biazzo, E. Brocato, L. Pulone, and L. Pasquini

2020 The Astronomical Journal 159 152.

Provider: AAS Journals

Caption: Figure 11.

Mean value of the logarithmic He abundance for each target. Error bars are also shown. The red dashed line represents the average of these values, while the yellow shadow region shows the ±1σ level.

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