Related papers: Monopolonium in confining phase

The paper has been withdrawn for further elaboration.

This paper has been withdrawn by the author due to the presented idea is wrong.

This paper has been withdrawn by the authors due to a crucial error in the proof of the main result. In a new manuscript (with two new authors) available at arXiv:1010.2791v1 this problem has been resolved.

This paper has been withdrawn by the authors due to new experimental results.

This paper has been withdrawn by the author because the conclusions reached in it are incorrect.

This paper has been withdrawn by the author(s),

This paper has been withdrawn temporarily.

This paper has been temprally withdrawn by the author

This paper has been withdrawn by the author due to a crucial mistakes.

This article has been withdrawn.

This paper is being withdrawn.

This paper has been withdrawn because the content has been substantially improved in a later paper, arXiv:0806.1165.

This paper has been withdrawn by the authors, because of serious experimental problems.

This paper has been withdrawn by the author. It will be posted on astro-ph once the proceedings of the 363rd Heraeus Seminar on Neutron Stars and Pulsars are ready.

This paper has been withdrawn by the author, since now all four parts of the review are available as a single file 0804.1639. I also made some revision of the text in order to avoid misprints and some inaccurate expressions.

This paper has been withdrawn by the author due to the fact that the results were found to be done previously.

This paper has been withdrawn by the author(s), due a crucial error in the data.

This paper has been withdrawn by the authors.

This paper has been withdrawn, because relevant publications, related to the subject of the paper, were overlooked by the author.

The paper has been withdrawn by the author.