射电浓度活性天体的红外发射
天体物理学
2007-05-23 v1
摘要
为了检验双束射电源的统一方案，研究了使用 ISOPHOT 对匹配样本中射电星系和射电浓度原子星的远红外特性。原子星数据 supplemented with nearly simultaneous 的亚毫米和厘米波射电数据。结果显示，原子星在远红外发射通常比射电星系更亮，且必须排除/beam/ 非热辐射作为解释红外过度的原因。然而，非热脉冲或光学厚的塔iki 仍可使结果与统一方案相一致。
引用
@article{arxiv.astro-ph/9902143,
title = {Infrared emission from radio-loud active nuclei},
author = {Ilse M. van Bemmel and Peter D. Barthel and Thijs de Graauw},
journal= {arXiv preprint arXiv:astro-ph/9902143},
year = {2007}
}
备注
4 pages including 1 figure, to be published in the proceedings of ESA conference 'The Universe as seen by ISO', ed. M. Kessler (ESA Special Publications series SP-427)