Interpretation of optical and IR light curves for transitional disk candidates in NGC 2264 using the extincted stellar radiation and the emission of optically thin dust inside the hole

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Bibliographic Details
Main Author:	E. Nagel
Format:	Artículo científico
Language:	en
Published:	Universidad Nacional Autónoma de México 2021
Subjects:	Física, Astronomía y Matemáticas Dust main sequence extinction stars: pre
Online Access:	Acceder al recurso 1 Acceder al recurso 2 Acceder al recurso 3 Acceder al recurso 4 Acceder al recurso 5
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