Semianalytical Accretion-tracer Emission: Forming Planets Are Intrinsically Faint
Authors: Gabriel-Dominique Marleau
Gabriel-Dominique Marleau
2026 The Astrophysical Journal1000.
Provider: AAS Journals
Caption: Figure 13.
Flow at two zoom levels for the same parameters as in Figure 1 (see description of elements there), but varying the relative centrifugal radius: fcent = 0.03 (left column; as in Figure 1) and fcent = 1/3 (right column).
