MESAS: Measuring the Emission of Stellar Atmospheres at Submm/mm wavelengths

26 Apr 2018 White Jacob Aaron Aufdenberg Jason Boley Aaron Hauschildt Peter Hughes A. Meredith Matthews Brenda Wilner David J.

In the early stages of planet formation, small dust grains grow to become mm sized particles in debris disks around stars. These disks can in principle be characterized by their emission at submillimeter and millimeter wavelengths... (read more)

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Categories


  • SOLAR AND STELLAR ASTROPHYSICS
  • EARTH AND PLANETARY ASTROPHYSICS