Related papers: Statistical studies of Galactic open clusters I. S…

This paper has been withdrawn due to a photometric calibration error.

This paper has been withdrawn by the authors due to an error.

The paper has been withdrawn because a new, substantially revised version of the theory of neutron star radiation is completed by the author.

The paper has been withdrawn by the author.

This paper has been withdrawn by the author because of publication in the journal Earth and Planetary Science Letters (Elsevier), which does not permit preprints at arxiv.org

This article has been removed. It has been superseded by gr-qc/0506097.

This paper has been withdrawn by the authors, because the authors have second thought that the new ideas in this paper are better to be contained in another paper.

This paper has been withdrawn by the author, due to errors in the figures.

This paper has been withdrawn by the author due to an error.

This paper has been withdrawn by the authors due to an unlikely results.

This paper is withdrawn by the authors

This paper has been withdrawn by the authors as requested by the journal.

This paper has been withdrawn. It was an early draft submitted prematurely in error. A complete version is to be submitted shortly.

This paper has been withdrawn by the author due to a gap in the proof of the main result.

This paper has been withdrawn by the author(s)!

This paper has been withdrawn by the author.

This paper has been withdrawn. A significantly revised version will be posted in the near future.

This paper has been withdrawn by the author due to a crucial sign error in equation 1.

This paper has been withdrawn by the author; see the much expanded, improved, and generalized version at arXiv:0811.2073.

This paper has been withdrawn by the author due to the paper does not belong to Condensed Matter field.