Possible variability of the magnetic field of T Tau
- Author
- SMIRNOV, D. A1 ; LAMZIN, S. A1 ; FABRIKA, S. N2 ; CHUNTONOV, G. A2 ; SAMUS, N (Translator)
[1] SternbergAstronomical Institute, Uniuersitetskii pr. 13, Moscow, 119992, Russian Federation
[2] Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, 357147 Karachai-Cherkessian Republic, Russian Federation - Source
Astronomy letters (Print). 2004, Vol 30, Num 7, pp 456-460, 5 p ; ref : 17 ref
- CODEN
- ALETEO
- ISSN
- 1063-7737
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Pleiades Publishing, New York, NY
- Publication country
- United States
- Document type
- Article
- Language
- Russian
- Keyword (fr)
- Champ magnétique Disque accrétion Etoile type T Tauri
- Keyword (en)
- Magnetic fields Accretion disks T Tauri stars
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C10 Stellar characteristics and properties / 001E03C10L Magnetic and electric fields. Polarization of starlight
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03C Stars / 001E03C21 Pre-main sequence objects, young stellar objects (yso's) and protostars (t tauri stars, orion population, herbig-haro objects, bok globules, bipolar outflows, cometary nebulae, etc.)
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 16032282
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
10.1134/1.1774397 
https://dx.doi.org/10.1134/1.1774397
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