相关论文: The Spectrum of HD 3651B: An Extrasolar Nemesis?
This paper was withdrawn. It has been superseded by the latest version of hep-th/0107069.
The paper was withdrawn due to another possible solution to the dataset that is significantly different in nature.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This paper has been withdrawn by the author(s), since it has been merged with paper I (astro-ph/0307482).
I present detailed analysis of the near infrared spectrum of HD 3651B, a faint, co-moving wide companion to the nearby planet-hosting star HD 3651. These data confirm the companion as a brown dwarf with spectral type T8, consistent with the…
This paper has been withdrawn. A significantly revised version will be posted in the near future.
A modified version of this paper is under process and with a new title and abstract. Hence, this version of the article is completely withdrawn.
The paper has been withdrawn
This paper has been withdrawn.
This paper has been withdrawn.
This paper has been withdrawn by the author.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 article has been removed. It has been superseded by gr-qc/0506097.
This paper has been withdrawn because the models on which it was based have undergone significant changes and improvements. A new paper with the same title, based on the improved models, is accepted for publication in MNRAS and is available…
This paper was withdrawn as it may have appeared elsewhere, although in a different form.
This paper has been withdrawn by the author(s), as it is superseded by 0708.2385.
%auto-ignore This paper has been withdrawn by the authors due to dublicate submission. To download the paper please go to astro-ph/0611081
This paper has been withdrawn.
This paper has been withdrawn by the authors.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.
This paper has been withdrawn.
This paper has been withdrawn by the authors after discussing its content with Dr. J. Madsen.
This paper has been withdrawn since its content is included in the more general version arXiv:0804.1882