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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 12.

log Teff − log g diagram for the stars analyzed spectroscopically by us with MUSE (black dots) and by other authors (magenta dots). The Z = 0.002 PARSEC isochrones of 18 and 30 Myr are also reported with red and blue solid lines, respectively. We also report the name of the stars. We show the log Teff and log g of A4 determined by us (A4) and by Lennon et al. (2003; A4L).

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