Disentangling interacting galaxy pairs and entangling them back

被引：0
|
作者：
Fuentes-Carrera, I. [1 ]
Amram, P. [2 ]
Balkowski, C. [1 ]
Flores, H. [1 ]
Puech, M. [1 ]
Yang, Y. [1 ]
Rosado, M. [3 ]
Hernandez-Toledo, H. [3 ]
机构：
[1] Univ Paris Diderot, CNRS, Observ Paris, GEPI, Pl Jules Janssen, F-92190 Meudon, France
[2] Lab Astrophys Marseille, 2 Pl Le Verrier, Marseille 4, France
[3] Univ Nacl Autonoma Mexico, Astron Inst, Apdo Postal 70264, Mexico City 04510, DF, Mexico
来源：
PATHWAYS THROUGH AN ECLECTIC UNIVERSE | 2008年 / 390卷
关键词：
D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Two-dimensional kinematics of disk galaxies give valuable information on the structure and evolution of these systems, complementing-sometimes contradicting-information derived from morphological studies. We present two cases of the use of two-dimensional kinematic information to study the interacting stage of galaxies. The first case portrays an apparently isolated local galaxy. The other points out the effects that higher redshifts-and thus the lack of spatial resolution-might have on the interpretation of this type of data.
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页码：186 / +
页数：2
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