Figure 4 from MUSE Observations of NGC330 in the Small Magellanic Cloud: Helium Abundance of Bright Main-sequence Stars

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 4.

Color–magnitude diagram of the selected stars in NGC 330. The isochrones at 10, 18, 30, and 50 Myr obtained from PARSEC (Bressan et al. 2012; Marigo et al. 2017) are overplotted with short green dashed, red solid, blue solid, and cyan short–long lines, respectively. The best-fitting isochrones are 18 Myr and 30 Myr.

Other Images in This Article

Copyright and Terms & Conditions