Related papers: Blue E/S0 galaxies: merger remnants or disk rebuil…

This paper has been withdrawn because the new one gr-qc/0512095 includes all its results (as well as those in gr-qc/0511016) in a clearer way.

This paper has been withdrawn by the authors due to overlap with other papers.

This paper was withdrawn as it may have appeared elsewhere, although in a different form.

This paper has been withdrawn by the author.

This paper has been withdrawn.

This paper has been withdrawn by the authors due to numerical problems to get viable results.

This paper has been withdrawn, because its material has been revised and became part of paper math.GT/0010184

The paper was withdrawn because of its significant overlap with a paper appeared recently.

This paper is withdrawn because it is a duplicate of astro-ph/0601311

This paper has been withdrawn by the author.

This paper has been withdrawn. Please see astro-ph/0502366.

This paper has been withdrawn by the authors. Significantly revised versions of the results of this paper are now available in arXiv:0707.0487v2 and arXiv:0808.3169v1.

The original version of this paper has been withdrawn by the authors and merged with the revised version of astro-ph/9702014.

This paper has been withdrawn.

We use numerical simulations to examine the structure of merger remnants resulting from collisions of gas-rich spiral galaxies. When the gas fraction of the progenitors is small, the remnants structurally and kinematically resemble…

The paper was withdrawn due to another possible solution to the dataset that is significantly different in nature. This issue will be addressed shortly and clarified with an additional data point.

This paper has been withdrawn by the author.

This paper has been withdrawn.

This article has been withdrawn; see astro-ph/0611542

This paper has been withdrawn by the authors, due to inappropriate discussions in Discussions.