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HST/GHRS Observations of Cool, Low-gravity Stars. VI. Mass-loss Rates and Wind Parameters for M Giants

  • Authors: Gioia Rau, Krister E. Nielsen, Kenneth G. Carpenter, and Vladimir Airapetian

2018 The Astrophysical Journal 869 1.

  • Provider: AAS Journals

Caption: Figure 1.

Hertzsprung–Russell diagram with evolutionary tracks from Marigo et al. (2013) for various stellar masses. Different colors indicate the location in the diagram of the various stars. γ Cru (⋆) and μ Gem (⋆), while the filled circles represent the comparison stars for the earlier papers in this program. A typical error bar is shown in the upper left side of the figure.

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