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Vol. 15 No. 1 (2003)
,
Contributions
Vol. 15 No. 1 (2003)
Contributions
Modeling the Dust Emission of the L 1551 IRS 5 Binary System at Different Scales
Osorio M.
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−
D'Alessio P.
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−
Muzerolle J.
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−
Calvet N.
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−
Hartmann L.
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−
Osorio M.
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA
D'Alessio P.
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Muzerolle J.
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Calvet N.
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Hartmann L.
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PDF
PDF
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
hola
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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.
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