测试银河系模型的偶极子与四极子矩
天体物理学
2009-10-28 v1
摘要
若伽马暴击中天体源自银河系，则其天空分布中应存在银河系模式。我们通过将已发表的银河系模型偶极子与四极子矩与 BATSE 3B 目录的矩进行比较，来检验这些模型。虽然许多模型的矩值过大，但仍有若干模型与数据在可接受或良好范围内一致。
引用
@article{arxiv.astro-ph/9610142,
title = {Testing the Dipole and Quadrupole Moments of Galactic Models},
author = {Michael S. Briggs and William S. Paciesas and Geoffrey N. Pendleton and Charles A. Meegan and Gerald J. Fishman and John M. Horack and Chryssa Kouveliotou and Dieter H. Hartmann and Jon Hakkila},
journal= {arXiv preprint arXiv:astro-ph/9610142},
year = {2009}
}
备注
5 pages, LaTex using Revtex macro aipbook.sty and psfig. To appear in the Proceedings of the 3rd Huntsville Symposium on Gamma-Ray Bursts, AIP, eds. C. Kouveliotou, M. S. Briggs, G. J. Fishman