Figure 5 from HST/GHRS Observations of Cool, Low-gravity Stars. VI. Mass-loss Rates and Wind Parameters for M Giants

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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 5.

Sample of SEI fits to lines representing a wide range of optical depths in the spectra of γ Cru. The full green line shows the GHRS observed spectrum; the red dotted line is the chromospheric profile input to the base of the wind; and the blue dashed line is the calculated profile.

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