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Semianalytical Accretion-tracer Emission: Forming Planets Are Intrinsically Faint

  • Authors: Gabriel-Dominique Marleau

Gabriel-Dominique Marleau 2026 The Astrophysical Journal 1000 .

  • Provider: AAS Journals

Caption: Figure 7.

Histograms of the luminosities from this work (red) and when converting ﹩{L}_{{\rm{acc}}}=G{M}_{{\rm{p}}}{\dot{M}}_{{\rm{Hill}},\,{\rm{net}}}/{R}_{{\rm{p}}}﹩ using scalings for CTTSs extrapolated down to planetary masses (J. M. Alcalá et al. 2017, consistent with the improved relations in E. Fiorellino et al. 2025; black) or scalings for planetary-mass objects (Y. Aoyama et al. 2021; blue). Left (right) panel: for Hα (Pa β).

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