后天习得 发表于 2025-3-28 17:22:24
http://reply.papertrans.cn/88/8707/870618/870618_41.png星球的光亮度 发表于 2025-3-28 20:29:43
Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena978-1-4020-2564-8Series ISSN 0067-0057 Series E-ISSN 2214-7985Budget 发表于 2025-3-29 00:34:48
http://reply.papertrans.cn/88/8707/870618/870618_43.png断言 发表于 2025-3-29 03:51:21
http://reply.papertrans.cn/88/8707/870618/870618_44.png进取心 发表于 2025-3-29 08:20:50
http://reply.papertrans.cn/88/8707/870618/870618_45.pngAntarctic 发表于 2025-3-29 15:26:37
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/s/image/870618.jpgWAG 发表于 2025-3-29 16:14:50
https://doi.org/10.1007/978-1-4020-2564-8Galaxy; Redshift; Universe; astronomy; stellarGLUE 发表于 2025-3-29 20:15:14
http://reply.papertrans.cn/88/8707/870618/870618_48.png含沙射影 发表于 2025-3-30 03:54:24
The Fuse Survey of O VI in the Galactic Halo including low and intermediate velocity H I, H. emission from the warm ionized gas at ~10. K, and hot X-ray emitting gas at ~40. K. The O VI has an average velocity dispersion, .=60 km s. and small standard deviation of 15 km s.. Thermal broadening alone cannot explain the large observed profile wieczema 发表于 2025-3-30 08:03:05
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