Figure 14 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 14.

He abundance versus distance from the center of NGC 330 for our MUSE sample. The dashed line represents the linear best fit to the data. The effective radius of NGC 330 is at 20″.

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