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Keywords

accretion
accretion disk
binaries: close
ISM: individual (L 1551 IRS 5)
radiative transfer
Stars: formation

How to Cite

Modeling the Dust Emission of the L 1551 IRS 5 Binary System at Different Scales. (2003). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 15(1), 142-142. https://astronomia.unam.mx/journals/rmxac/article/view/2003rmxac..15..142o
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Abstract

We present a self-consistent model to investigate the physical properties on different scales of the circumstellar material around the Class I source L 1551 IRS 5.