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Data sources: Datacite
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Understanding Balmer decrements in CTTS using two-flow magnetospheric accretion - Figures

appsOther research productkeyboard_double_arrow_right Image 28 Oct 2025Publisher:Zenodo
Authors: Patiño, Naiara; Calvet, Nuria; Magris, Gladis; Micolta, Marbely; Waters, Thomas; Thanathibodee, Thanawuth; Colmenares Diaz, Maria Jose;

doi: 10.5281/zenodo.17460555 , 10.5281/zenodo.17460554

Understanding Balmer decrements in CTTS using two-flow magnetospheric accretion - Figures

Abstract

Collection of figures from "Understanding Balmer Decrements in T Tauri stars in terms of Multi-column MagnetosphericAccretion". 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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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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