在附近的晚型星系周围检测到马射线光
1Russian Academy of Sciences, Institute for Nuclear Research, Lomonosov Moscow State University, Sternberg Astronomical Institute, Universitetsky prospekt 13, 119992, Moscow, Russia and , Prospekt 60-letiya Oktyabrya, 7a, 117312, Moscow, Russia.
Physical review letters
|March 13, 2026
概括
研究人员在附近的星系周围发现了扩展的马射线光环,这表明宇宙射线相互作用而不是暗物质. 这一发现为银河系排放和环银河系介质提供了新的见解.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- 宇宙学的宇宙学是什么?
背景情况:
- 理论模型预测星系周围扩展的马射线光环.
- 这些光环可能源于宇宙射线相互作用或暗物质粒子毁灭/衰变.
- 对安德罗米达星 (M31) 的观测证实了这种光环的存在.
研究的目的:
- 搜索来自15Mpc以内的星系的马射线辐射,能量>2GeV.
- 为了确定这个辐射的空间延伸.
- 要区分宇宙射线相互作用和暗物质作为源.
主要方法:
- 使用了局部星系目录和光圈光度学.
- 应用质量,能量和空间选择标准来识别目标星系.
- 员工进行了堆叠概率分析,以证实调查结果.
主要成果:
- 从16个晚型星系中检测到统计学上显著的马射线过量 (p值3.7x10^-7).
- 过量源于一个扩展源 (半径~0.3°,~80 kpc物理半径),而不是一个点源.
- 从六个早期类型星系中没有发现任何显著的过剩.
结论:
- 扩展的马射线辐射更可能是由于宇宙射线与环银河系介质的相互作用.
- 这些发现有利于宇宙射线相互作用而不是暗物质毁灭/衰变.
- 不规则的形状和晚期类型的星系协会表明星系特定的过程影响光环形成.
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