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Hydrogen-line Emission in Accreting Low-mass Objects. I. Spectral Analysis of Shock-origin Narrow Component

  • Authors: Yuhiko Aoyama, Jun Hashimoto, Gabriel-Dominique Marleau, Carlo F. Manara, Juan Manuel Alcalá, Gregory Herczeg, Camille Bergez-Casalou, Masahiro Ikoma

Yuhiko Aoyama et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

Schematic illustration of magnetospheric accretion and accretion shock. In this paper, “shock emission” refers to emission from the shock-heated gas (orange). Emission from the accretion column and/or disk wind is referred to as “nonshock emission.”

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