Measured Mass-Loss Rates of Solar-like Stars as a Function of Age and Activity

@article{Wood2002MeasuredMR,
  title={Measured Mass-Loss Rates of Solar-like Stars as a Function of Age and Activity},
  author={Brian E. Wood and H. R. Mueller and Gary P. Zank and Jeffrey L. Linsky},
  journal={The Astrophysical Journal},
  year={2002},
  volume={574},
  pages={412 - 425}
}
Collisions between the winds of solar-like stars and the local interstellar medium result in a population of hot hydrogen gas surrounding these stars. Absorption from this hot H I can be detected in high-resolution Lyα spectra of these stars from the Hubble Space Telescope. The amount of absorption can be used as a diagnostic for the stellar mass-loss rate. We present new mass-loss rate measurements derived in this fashion for four stars (ϵ Eri, 61 Cyg A, 36 Oph AB, and 40 Eri A). Combining… 

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