Related papers: PSR B1929+10 Revisited in X-Rays

This paper has been withdrawn, as it should not have been a new submission. Please instead see the latest version of arXiv:0904.0436.

This manuscript has been withdrawn by the author. Some of the material has been included in the manuscript 'Embedded Monopoles' at hep-th/0106254.

This paper has been withdrawn by the author.

This paper has been withdrawn by the author due to the presented idea is wrong.

This paper has been withdrawn, since it contains a corollary with impossible consequences and the source of an error is currently unknown.

The paper has been withdrawn.

This paper has been withdrawn: it has been merged with the preprint to which it refers.

This paper has been withdrawn by the author.

This paper has been withdrawn by the authors because the paper is largely revised and improved, and to appear in Mechanics Research Communications.

This submission has been withdrawn by arXiv administrators due to misrepresentation of authorship.

This paper has been withdrawn by the author, due to errors in the figures.

This paper has been withdrawn by the authors. due fail of replacement of the paper. new version is hep-ph/0201214.

This paper has been withdrawn for extensive revision.

This paper has been withdrawn by the authors.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The paper has been withdrawn because a new, substantially revised version of the theory of neutron star radiation is completed by the author.

This paper is being withdrawn.

This paper has been withdrawn by the author, due to a significant error in section 4.3.1.

This paper has been withdrawn by the author.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.

The paper has been withdrawn

This paper has been withdrawn by the author.