A Model of the C iv λ λ1548, 1550 Doublet Line in T Tauri Stars

A Model of the C iv λ λ1548, 1550 Doublet Line in T Tauri Stars

The C iv doublet in the UV has long been associated with accretion in T Tauri stars. However, it is still unclear where and how the lines are formed. Here, we present a new C iv line model based on the currently available accretion shock and accretion flow models. We assume axisymmetric, dipolar acc...

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Bibliographic Details
Main Authors: Thanawuth Thanathibodee, Connor E. Robinson, Nuria Calvet, Catherine C. Espaillat, Caeley V. Pittman, Nicole Arulanantham, Kevin France, Hans Moritz Günther, Seok-Jun Chang, P. Christian Schneider
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
T Tauri stars
Stellar accretion
Ultraviolet astronomy
Protoplanetary disks
Astronomical models
Radiative transfer
Online Access:https://doi.org/10.3847/1538-4357/ad7b2d

Internet

https://doi.org/10.3847/1538-4357/ad7b2d

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