“星系中的射电辐射”的版本间差异

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星系中的射电辐射主要有三种
星系中的射电辐射主要有三种


#同步辐射 (低频,幂律谱)
*同步辐射 (低频,幂律谱)
#自由-自由散射 (HII区:低频是接近于热谱,光学厚,高频光学薄,平谱)
*自由-自由散射 (HII区:低频是接近于热谱,光学厚,高频光学薄,平谱)
:https://www.cv.nrao.edu/course/astr534/FreeFreeEmission.html
:https://www.cv.nrao.edu/course/astr534/FreeFreeEmission.html
#AME
*AME
:Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10–60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997
:Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10–60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997

==恒星形成相关==
* 射电与光学观测的关系(恒星形成)Radio-dim and bright regions in spiral galaxies [https://arxiv.org/abs/2307.09154]

2023年7月19日 (三) 09:21的最新版本

星系中的射电辐射主要有三种

  • 同步辐射 (低频,幂律谱)
  • 自由-自由散射 (HII区:低频是接近于热谱,光学厚,高频光学薄,平谱)
https://www.cv.nrao.edu/course/astr534/FreeFreeEmission.html
  • AME
Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10–60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997

恒星形成相关

  • 射电与光学观测的关系(恒星形成)Radio-dim and bright regions in spiral galaxies [1]