Light curve variation caused by accretion column switching stellar hemispheres

I use two-dimensional axisymmetric numerical simulations of star-disk magnetospheric interaction to construct a three-dimensional model of hot spots on the star created by infalling accretion columns. The intensity of emitted radiation is computed with minimal assumptions, as seen by observers at in...

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Veröffentlicht in:	arXiv.org 2018-11
1. Verfasser:	Čemeljić, Miljenko
Format:	Artikel
Sprache:	eng
Schlagworte:	Angles (geometry) Computer simulation Deposition Hemispheres Light curve Magnetospheres Mathematical models Parameter modification Physical properties Physics - Solar and Stellar Astrophysics Three dimensional models
Online-Zugang:	Volltext
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