POSSIBLE PRECESSION MOTION IN THE BIPOLAR PROTO-PLANETARY NEBULA IRAS 17441-2411
- Author
- VOLK, Kevin1 ; KWOK, Sun2 ; HRIVNAK, Bruce J3 4
[1] Gemini Observatory, Hilo, United States
[2] University of Hong Kong, Hong-Kong
[3] Department of Physics and Astronomy, University of Calgary, Calgary, AB T2N 1N4, Canada
[4] Department of Physics and Astronomy, Valparaiso University, Valparaiso, IN 46383, United States - Source
The Astrophysical journal. 2007, Vol 670, Num 2, pp 1137-1141, 5 p ; 1 ; 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
- circumstellar matter infrared: stars planetary nebulae: general stars: AGB and post-AGB
- Keyword (fr)
- Branche géante asymptotique Etoile IR Matière circumstellaire Nébuleuse bipolaire Nébuleuse planétaire Nébuleuse proto planétaire Précession
- Keyword (en)
- Asymptotic giant branch Infrared star Circumstellar matter Bipolar nebula Planetary nebulae Proto planetary nebula Precession
- Keyword (es)
- Rama gigante asintótica Estrella IR Nebulosa bipolar Nebulosa proto planetaria
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19893250
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
10.1086/522225 
https://dx.doi.org/10.1086/522225
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