SINFONI adaptive optics integral field spectroscopy of the Circinus Galaxy
- Author
- MUELLER SANCHEZ, F1 ; DAVIES, R. I1 ; EISENHAUER, F1 ; TACCONI, L. J1 ; GENZEL, R1 2 ; STERNBERG, A3
[1] Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse, Postfach 1312, 85741 Garching, Germany
[2] Department of Physics, 366 Le Conte Hall, University of California, Berkeley, CA, 94720-7300, United States
[3] School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978, Israel - Source
Astronomy and astrophysics (Berlin. Print). 2006, Vol 454, Num 2, pp 481-492, 12 p ; ref : 44 ref
- 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
- galaxies: Seyfert galaxies: active galaxies: individual: Circinus galaxies: nuclei galaxies: starburst infrared: galaxies
- Keyword (fr)
- Activité stellaire Champ proche Cinématique Continuum Densité colonne Dynamique gaz Dynamique stellaire Epaisseur optique Formation stellaire Galaxies Seyfert Galaxies actives Galaxies infrarouges Galaxies à flambée Luminosité Modèle Morphologie Noyau galactique actif Noyau galaxies Optique adaptative Profil raie Propriété physique Raie coronale Spectrométrie Tore
- Keyword (en)
- Stellar activity Near field Kinematics Continuum Column density Gas dynamics Stellar dynamics Optical thickness Star formation Seyfert galaxies Active galaxies Infrared galaxies Starburst galaxies Luminosity Models Morphology Active galaxy nuclei Galaxy nuclei Adaptive optics Line shape Physical properties Coronal line Spectroscopy Tori
- Keyword (es)
- Campo próximo Continuo Densidad columna Espesor óptico Galaxias infrarrojas Galaxias llamarada estelar Modelo Raya coronal
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 17979597
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
10.1051/0004-6361:20054387 
https://dx.doi.org/10.1051/0004-6361:20054387
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