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Prospects for Life on Temperate Planets around Brown Dwarfs

  • Authors: Manasvi Lingam, Idan Ginsburg, and Abraham Loeb

2020 The Astrophysical Journal 888 102.

  • Provider: AAS Journals

Caption: Figure 5.

The wavelength λpeak (in μm) at which the maximal value of the brown dwarf’s photon flux density occurs plotted as a function of its age. The dotted, unbroken, and dashed black curves depict λpeak for brown dwarfs whose masses are 10 MJ, 40 MJ, and 70 MJ, respectively.

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