AAS Journals
Published October 28, 2025 | Version v1
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Understanding Balmer decrements in CTTS using two-flow magnetospheric accretion - Figures

Authors/Creators

  • 1. ROR icon Boston University
  • 2. ROR icon University of Michigan–Ann Arbor
  • 3. Centro de Investigaciones de Astronomía, CIDA
  • 4. ROR icon Chulalongkorn University

Description

Collection of figures from "Understanding Balmer Decrements in T Tauri stars in terms of Multi-column Magnetospheric
Accretion".

 

fits_twocolumn_all.pdf: Fits to observed Balmer fluxes for CTTS of Lupus, Chamaleon I, Orion OB1b and Upper Scorpius using two-column accretion model. Continuous lines correspond to the measured fluxes of 1000 models randomly extracted from the final, post-burn-in MCMC sample after 10,000 steps. Scatter points correspond to the dereddened measured fluxes from CTTS of each region.

corner_twocolumn.pdf.zip: Corner plots with parameter distributions of MCMC samples shown in fits_twocolumn_all.pdf

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cornerplots_twocolumn.pdf.zip

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