| Lien | http://aspbooks.org/custom/publications/paper/317-0279.html |
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| Auteur | Rechercher : Foster, T.1; Rechercher : Routledge, D.1 |
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| Affiliation | - Conseil national de recherches Canada. Institut Herzberg d'astrophysique du CNRC
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| Format | Texte, Article |
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| Conférence | The 5th Boston University Astrophysics Conference, 15-17 June 2003, Boston, MA, USA |
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| Résumé | Models of the smooth large-scale radial distribution of the column depth of H I in the thin disk are used to found a new technique of mapping the velocity field of the Outer Galaxy in the second quadrant. The results show common features across this quadrant: a) locally (r ≤ 2 kpc), Galactic H I obeys a flat rotation law (with R0=8 kpc & v0=220 km s−1) b) beyond r=2 kpc, velocities of H I in the plane (|b| ≤ 5° ) show pronounced deviation from velocity fields predicted by flat circular rotation, and c) towards relatively high latitudes (|b| > 5° ), the Galactic H I exhibits “normal” behavior, with observed velocities congruent with those predicted by flat circular rotation. |
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| Date de publication | 2004 |
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| Dans | |
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| Série | |
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| Langue | anglais |
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| Numéro NPARC | 9720627 |
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| Exporter la notice | Exporter en format RIS |
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| Signaler une correction | Signaler une correction (s'ouvre dans un nouvel onglet) |
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| Identificateur de l’enregistrement | d215ba88-2225-4e2b-8db2-dfda7b4d7be2 |
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| Enregistrement créé | 2009-07-17 |
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| Enregistrement modifié | 2020-04-17 |
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