$m{H}alpha$ Velocity Fields and Galaxy Interaction in the Quartet of Galaxies NGC 7769, 7770, 7771 and 7771A

Journal of astrophysics and astronomy

T. A. Nazaryan1¹  A. A. Hakobyan1¹  A. A. Yeghiazaryan¹ 

[1] Byurakan Astrophysical Observatory, 0213 Byurakan, Aragatsotn Province, Armenia.$$

关键词: Galaxies: interactions;    galaxies: star formation;    galaxies: peculiar;    galaxies: individual: NGC 7769;    NGC 7770;    NGC 7771;    NGC 7771A;    supernovae: individual: 2003hg;   

DOI  :  

学科分类：天文学(综合)

来源: Indian Academy of Sciences

【 摘 要 】

The quartet of galaxies NGC 7769, 7770, 7771 and 7771A is a system of interacting galaxies. Close interaction between galaxies caused characteristic morphological features: tidal arms and bars, as well as an induced star formation. In this study, we performed the Fabry–Perot scanning interferometry of the system in $m{H}alpha$ line and studied the velocity fields of the galaxies. We found that the rotation curve of NGC 7769 is weakly distorted. The rotation curve of NGC 7771 is strongly distorted with the tidal arms caused by direct flyby of NGC 7769 and flyby of a smaller neighbor NGC 7770. The rotation curve of NGC 7770 is significantly skewed because of the interaction with the much massive NGC 7771. The rotation curves and morphological disturbances suggest that the NGC 7769 and NGC 7771 have passed the first pericenter stage, however, probably the second encounter has not happened yet. Profiles of surface brightness of NGC 7769 have a characteristic break, and profiles of color indices have a minimum at a radius of intensive star formation induced by the interaction with NGC 7771.

【 授权许可】

Unknown