STRONG NEAR-INFRARED EMISSION INTERIOR TO THE DUST SUBLIMATION RADIUS OF YOUNG STELLAR OBJECTS MWC 275 AND AB AURIGAE
- Author
- TANNIRKULAM, A1 ; MONNIER, J. D1 ; MILLAN-GABET, R2 ; HARRIES, T. J3 ; PEDRETTI, E4 ; TEN BRUMMELAAR, T. A5 ; MCALISTER, H5 ; TURNER, N5 ; STURMANN, J5 ; STURMANN, L5
[1] University of Michigan, Astronomy Department, 500 Church Street, 1017 Dennison Building, Ann Arbor, MI 48109-1042, United States
[2] Michelson Science Center, Pasadena, CA, United States
[3] University of Exeter, School of Physics, Stocker Road, Exeter EX4 4QL, United Kingdom
[4] University of St. Andrews, Scotland, United Kingdom
[5] CHARA, Georgia State University, Atlanta, GA, United States - Source
The Astrophysical journal. 2008, Vol 677, Num 1 ; L51-L54 ; 2 ; ref : 1/4 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- planetary systems: protoplanetary disks-radiative transfer-stars: pre-main-sequence- techniques: interferometric
- Keyword (fr)
- Nébuleuse proto planétaire Objet stellaire jeune Sublimation Système planétaire Transfert radiatif
- Keyword (en)
- Proto planetary nebula Young stellar object Sublimation Planetary system Radiative transfer
- Keyword (es)
- Nebulosa proto planetaria Objeto estelar joven Sistema planetario
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20271347
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1086/587873 
https://dx.doi.org/10.1086/587873
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