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arXiv · astro-ph/9903096

Formation of massive counter-rotating disks: an alternative scenario

I. Puerari·D. Pfenniger
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Abstract

In this contribution, we investigate the scenario of major mergers between galaxies of comparable mass to the formation of massive counter-rotating disks. Such a scenario can be ruled out in general because they produce rather ellipticals. Yet for a narrow range of initial conditions, major mergers can nevertheless produce anyway rare galaxies such as NGC 4550, and so they are viable alternatives for the formation of these counter-rotating systems. The scenario is successful in producing a remarkably axisymmetric disk possessing strongly counter-rotating populations.

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I. Puerari, D. Pfenniger. 1999-03-06. Formation of massive counter-rotating disks: an alternative scenario. https://doi.org/10.1023/a%3A1017581325673

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