Mereghetti, S. 2009 磁星SGR 1627-41 and 1E 1547-5408
主要内容:
这两个源有些类似的性质, 可能说明Anomalous X–ray Pulsars and Soft Gamma-ray Repeaters是同一类磁星.
精彩摘抄:
文章信息:
· Find Similar Abstracts (with default settings below) - · arXiv e-print (arXiv:0908.0414)
- · References in the Article
- ·
- · Translate This Page
Title: | The Twin Magnetars: SGR 1627-41 and 1E 1547-5408 | |
Authors: | Mereghetti, S.; Tiengo, A.; Esposito, P.; Vianello, G.; De Luca, A.; Gotz, D.; Weidenspointner, G.; von Kienlin, A.; Israel, G. L.; Stella, L.; Rea, N.; Turolla, R.; Zane, S. | |
Publication: | eprint arXiv:0908.0414 | |
Publication Date: | 08/2009 | |
Origin: | ARXIV | |
Keywords: | Astrophysics - High Energy Astrophysical Phenomena | |
Comment: | To be published in the proceedings of the conference "Neutron Stars and Gamma Ray Bursts: Recent Developments and Future Directions" - March 30 - April 4, 2009 (Cairo and Alexandria, Egypt) | |
Bibliographic Code: | 2009arXiv0908.0414M |
Abstract
We report on recent results obtained thanks to Target of Opportunity observations of the two galactic sources SGR 1627-41 and 1E 1547-5408. These two transient sources present several similarities which support the interpretation of Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters as a single class of strongly magnetized neutron stars.Bibtex entry for this abstract Preferred format for this abstract (see Preferences)
没有评论:
发表评论