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

This paper is withdrawn because the results in the paper are included in a paper to be published in Mathematical and Computer Modelling.

This article has been withdrawn due to an error in a proof of the main result.

This paper has been withdrawn by the author. It will be replaced, substantially modified, by sections of the author's completed PhD thesis.

This submission has been withdrawn by arXiv administrators because it is a duplicate of astro-ph/0701570.

This paper has been withdrawn by the authors because it has been merged with paper arXiv:0903.3501v1 [math.DG]

This paper as been withdrawn. This paper as been withdrawn. This paper as been withdrawn. This paper as been withdrawn. This paper as been withdrawn. This paper as been withdrawn.

This paper has been withdrawn by the author due to an error

This article has been withdrawn; see astro-ph/0611542

This paper has been retracted, for obvious reasons.

This paper has been withdrawn by the authour.

This paper has been withdrawn by the authors, because of serious experimental problems.

This paper has been withdrawn by the authors

This paper has been withdrawn. The contents of this paper can now be found in 0907.3000, which combines the erstwhile 0901.2981 and 0901.2982 in a somewhat compact form.

This paper has been withdrawn to allow publication elsewhere.

This paper has been withdrawn by the author due to an error.

The paper is withdrawn due to certain inherent problem in the public archival data of BATSE which may have modulation due to satellite precession.

This paper has been withdrawn by the author, due to errors in the figures.

This paper has been withdrawn by the authors due to need of essential revision.

This paper has been withdrawn by the authors. We have discovered an error in the evaluation of the diagram, which invalidates our conclusion.

This paper has been withdrawn because its contents have become subsumed in Section 5.2 of arXiv:0805.2307.