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Indications of Rapid Dust Formation in the Inner Region of a Protoplanetary Disk

  • Authors: Thanawuth Thanathibodee, Catherine Espaillat, Nuria Calvet, Zhaohuan Zhu, Julalak Nammanee, Caeley Pittman, Máire Volz

Thanawuth Thanathibodee et al 2026 The Astrophysical Journal Letters 999 .

  • Provider: AAS Journals

Caption: Figure 4.

Hα profiles of CVSO 1942 across 15 yr. The blue lines represent the observations, the red lines represent the average magnetospheric model, and the gray lines represent the top 100 best-fit models. The orange lines are the average chromospheric models, and the black lines are the average total models.

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