Monomania 发表于 2025-3-21 17:54:24
书目名称Galactic Astrophysics and Gamma-Ray Astronomy影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0380328<br><br> <br><br>书目名称Galactic Astrophysics and Gamma-Ray Astronomy读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0380328<br><br> <br><br>insurrection 发表于 2025-3-21 23:44:47
Kathy Lee-Son,Massimo Attanasio in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were lively — sometimes heated — and the original time span allocated to the meeting was a result, comfortably exceeded by about 50%.inhibit 发表于 2025-3-22 01:25:57
http://reply.papertrans.cn/39/3804/380328/380328_3.pngGROUP 发表于 2025-3-22 07:09:05
http://reply.papertrans.cn/39/3804/380328/380328_4.pngHighbrow 发表于 2025-3-22 12:42:21
https://doi.org/10.1007/978-1-4613-4024-9ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hump is discussed.periodontitis 发表于 2025-3-22 14:42:49
http://reply.papertrans.cn/39/3804/380328/380328_6.pngperiodontitis 发表于 2025-3-22 17:19:08
Cosmic Gamma Rays and Molecular Gas in the Galaxy,It is shown that, locally, γ-ray data enable the calibration of H. densities to be inferred from CO data and elsewhere the variation of cosmic-ray intensity with position to be assessed. Finally, the importance of cosmic-ray irradiated molecular clouds in simulating γ-ray ‘sources’ is reiterated.织物 发表于 2025-3-22 23:31:44
http://reply.papertrans.cn/39/3804/380328/380328_8.png山顶可休息 发表于 2025-3-23 02:42:44
Comparison of Far-Infrared Radiation with Gamma Radiation,ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hump is discussed.accomplishment 发表于 2025-3-23 09:26:40
http://reply.papertrans.cn/39/3804/380328/380328_10.png