Rotating halos and spirals in low surface brightness galaxies

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/34107

Title:	Rotating halos and spirals in low surface brightness galaxies
Authors:	Chiueh,T;Tseng,YH
Contributors:	天文研究所
Keywords:	DARK-MATTER HALOES;ANGULAR-MOMENTUM;BARRED GALAXIES;TIDAL TORQUES;DISK GALAXIES;EVOLUTION;SHAPES;INSTABILITY;CLUSTERS;WARPS
Date:	2000
Issue Date:	2010-07-07 11:57:34 (UTC+8)
Publisher:	中央大學
Abstract:	As the angular momentum of visible matter in a spiral galaxy is derived from the host cloud, the dark matter halo left behind in the cloud is likely to be in rotation also. In the merging model of galaxy formation, it is shown that the conservation of mas
Relation:	ASTROPHYSICAL JOURNAL
Appears in Collections:	[Graduate Institute of Astronomy] journal & Dissertation

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