Peculiar velocities of field spiral galaxies near and beyond the Great Attractor
- Author
- BOTHUN, G. D1 ; SCHOMMER, R. A; WILLIAMS, T. B; MOULD, J. R; HUCHRA, J. P
[1] Univ. Oregon, dep. physics, Eugene OR 97403, United States - Source
The Astrophysical journal. 1992, Vol 388, Num 2, pp 253-267 ; p.1 ; ref : 1/2 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
- Keyword (fr)
- Courbe rotation Distance Dynamique stellaire Déplacement vers le rouge Etude comparative Galaxies spirales Galaxies type avancé Modèle Mécanique céleste Observation spectroscopique Vitesse Grand Attracteur Relation Tully Fisher
- Keyword (en)
- Rotation curve Distance Stellar dynamics Redshift Comparative study Spiral galaxies Late type galaxies Models Celestial mechanics Spectroscopical observation Velocity Great Attractor Tully Fisher relation
- Keyword (es)
- Curva rotación Distancia Dinámica estelar Desplazamiento hacia el rojo Estudio comparativo Galaxias espirales Galaxias tipo avanzado Modelo Mecánica celeste Observación espectroscópica Velocidad Gran Atractor Relación Tully Fisher
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D62 Characteristics and properties of external galaxies and extragalactic objects / 001E03D62P Distances, redshifts, radial velocities. Spatial distribution of galaxies
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 5169677
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
10.1086/171149 
https://dx.doi.org/10.1086/171149
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