Spectral imaging of the Sagittarius B2 region in multiple 3-mm molecular lines with the Mopra telescope
- Author
- JONES, P. A1 ; BURTON, M. G1 ; CUNNINGHAM, M. R1 ; MENTEN, K. M2 ; SCHILKE, P2 ; BELLOCHE, A2 ; LEURINI, S3 ; OTT, J4 5 ; WALSH, A. J6
[1] School of Physics, University of New South Wales, NSW 2052, Australia
[2] Max-Planck-Institut für Radioastronomie, Aufdem Hügel 69, 53121 Bonn, Germany
[3] European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany
[4] National Radio Astronomy Observatory, 520 Edgemont Road, Charlottesville, VA 22903, United States
[5] California Institute of Technology, 1200 E. California Blvd, Pasadena, CA 91125-2400, United States
[6] School of Maths, Physics and IT, James Cook University, Qld4814, Australia - Source
Monthly Notices of the Royal Astronomical Society. 2008, Vol 386, Num 1, pp 117-137, 21 p ; ref : 3/4 p
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Blackwell Science, Oxford
- Publication country
- United Kingdom
- Document type
- Article
- Language
- English
- Author keyword
- ISM: individual: Sagittarius B2 ISM: kinematics and dynamics ISM: molecules radio lines: ISM
- Keyword (fr)
- Abondance Carte radio Cinématique Continuum Cyanure d'hydrogène Densité colonne Dynamique Excitation Noyau stellaire Position
- Keyword (en)
- Abundance Radio map Kinematics Continuum Hydrogen cyanides Column density Dynamics Excitation Stellar cores Positions
- Keyword (es)
- Mapa radio Continuo Hidrogeno cianuro Densidad columna
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20291905
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
10.1111/j.1365-2966.2008.13009.x 
https://dx.doi.org/10.1111/j.1365-2966.2008.13009.x
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