Fitting Balmer fluxes of CTTS using two-column magnetospheric accretion
Authors/Creators
-
1.
Boston University
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2.
University of Michigan–Ann Arbor
- 3. Centro de Investigaciones de Astronomía, CIDA
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4.
University of Michigan
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5.
Chulalongkorn University
Description
Collection of figures from "Understanding Balmer Decrements in T Tauri stars in terms of Multi-column Magnetospheric
Accretion" (Patiño et al. in prep).
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
fits_twocolumn_filtered.pdf: Same as fits_twocolumn_all.pdf but filtered by excluding objects with high chromospheric contribution
fits_twocolumn_high_chrom.pdf: Same as fits_twocolumn_all.pdf but only including objects with high chromospheric contribution
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