A search for near-infrared molecular hydrogen emission in the CTTS LkHa 264 and the debris disk 49 Ceti
- Author
- CARMONA, A1 2 ; VAN DEN ANCKER, M. E2 ; HENNING, Th1 ; GOTO, M1 ; FEDELE, D2 3 ; STECKLUM, B4
[1] Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
[2] European Southern Observatory, Karl Schwarzschild Strasse 2, 85748 Garching bei München, Germany
[3] Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
[4] Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany - Source
Astronomy and astrophysics (Berlin. Print). 2007, Vol 476, Num 2, pp 853-862, 10 p ; ref : 3/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- stars: emission-line, Be stars: planetary systems: protoplanetary disks stars: pre-main sequence
- Keyword (fr)
- Borne supérieure Etoile pré séquence principale Etoile raie émission Etoile type T Tauri Excès UV Modélisation Molécule d'hydrogène Nébuleuse proto planétaire Optique adaptative Profil raie Propriété physique Raie H alpha Système planétaire
- Keyword (en)
- Upper bound Pre-main-sequence stars Emission line stars T Tauri stars Ultraviolet excess Modelling Hydrogen molecules Proto planetary nebula Adaptive optics Line shape Physical properties H-alpha lines Planetary system
- Keyword (es)
- Cota superior Exceso UV Nebulosa proto planetaria Sistema planetario
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19868904
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
10.1051/0004-6361:20078536 
https://dx.doi.org/10.1051/0004-6361:20078536
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