The nature of the high-velocity gas in NGC 1275: first results with TAURUS-2 on the William Herschel telescope
- Auteur
- UNGER, S. W1 ; TAYLOR, K; PEDLAR, A; GHATAURE, H. S; PENSTON, M. V; ROBINSON, A
[1] Royal Greenwich obs., Hailsham East Sussex BN27 1RP, United Kingdom - Source
Monthly Notices of the Royal Astronomical Society. 1990, Vol 242, Num 2, pp 33P-39P ; ref : 49 ref
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Domaine scientifique
- Astronomy earth cosmic environment
- Editeur
- Blackwell Science, Oxford
- Pays de publication
- United Kingdom
- Type de document
- Article
- Langue
- English
- Mot clé (fr)
- Carte radio Distribution vitesse Galaxies actives Gaz interstellaire Grande vitesse Imagerie Instrumentation Intensité Observation interférométrique Raie Hα Raie émission NGC 1275 TAURUS-2
- Mot clé (en)
- Radio map Velocity distribution Active galaxies Interstellar gas High speed Imagery Instruments Intensity Interferometric observation Hα line Emission line
- Mot clé (es)
- Mapa radio Distribución velocidad Galaxias activas Gas interestelar Gran velocidad Imaginería Instrumentación Intensidad Observación interferométrica Raya Hα Raya emisión
- Classification
- Pascal
- 001 Sciences exactes et technologie / 001E Terre, ocean, espace / 001E03 Astronomie / 001E03D Systèmes stellaires. Objets et systèmes galactiques et extragalactiques. L'univers / 001E03D54 Quasars. Systèmes, objets et galaxies actives ou particulières
- Discipline
- Astronomy
- Provenance
- Inist-CNRS
- Base de données
- PASCAL
- Identifiant INIST
- 6789258
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
10.1093/mnras/242.1.33P 
https://dx.doi.org/10.1093/mnras/242.1.33P
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