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Ultraviolet Accretion Continua Reveal a Transition in T Tauri Magnetic Topology

  • Authors: Ana I. Gómez de Castro

Ana I. Gómez de Castro 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 3.

Empirical UV photospheric sequence and photosphere-plus-shock model envelope. Warm TTSs (G0–K5; red circles), late-type TTSs (K6–M5; blue squares), and main-sequence stars (gray triangles) are shown in the ﹩\mathrm{log}(F270/F303)﹩–spectral-type plane. The solid blue curve represents the empirical photospheric sequence derived from the main-sequence sample. The shaded region shows the range of UV colors spanned by the adopted ensemble of photosphere-plus-shock models for veiling factors R = 0.01–0.5.

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