Figure 13 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 13.

log T_eff − log g diagram for the stars analyzed spectroscopically by us with MUSE (black dots) considering stellar rotation. The Z = 0.002 SYCLIST isochrones of 30 Myr and ω = 0.9ω_c (Georgy et al. 2014) is reported with the red solid line. We report also the names of the stars.

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