Taft
发表于 2025-3-21 17:06:50
书目名称Cosmic Rays in Star-Forming Environments影响因子(影响力)<br> http://impactfactor.cn/2024/if/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments影响因子(影响力)学科排名<br> http://impactfactor.cn/2024/ifr/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments网络公开度<br> http://impactfactor.cn/2024/at/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments网络公开度学科排名<br> http://impactfactor.cn/2024/atr/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments被引频次<br> http://impactfactor.cn/2024/tc/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments被引频次学科排名<br> http://impactfactor.cn/2024/tcr/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments年度引用<br> http://impactfactor.cn/2024/ii/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments年度引用学科排名<br> http://impactfactor.cn/2024/iir/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments读者反馈<br> http://impactfactor.cn/2024/5y/?ISSN=BK0238898<br><br> <br><br>书目名称Cosmic Rays in Star-Forming Environments读者反馈学科排名<br> http://impactfactor.cn/2024/5yr/?ISSN=BK0238898<br><br> <br><br>
拥挤前
发表于 2025-3-21 21:14:03
Martina Zeleňáková,Abdelazim M. Negmexternal galaxies. We will review the methodologies employed to determine the cosmic ray ionization rates in the ISM, how cosmic rays rates can influence the determination of the mass of a galaxy and, finally, how cosmic rays affect star formation and its rate.
畏缩
发表于 2025-3-22 02:31:42
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Explosive
发表于 2025-3-22 04:33:15
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BIBLE
发表于 2025-3-22 10:57:20
D. Káposztásová,Z. Vranayová,P. Purczl stellar radiation propagating through the dusty ISM of galaxies. It is in such CR-dominated regions (CRDRs) rather than Photon-dominated regions (PDRs) of H. clouds where the star formation initial conditions are set, making CRs the ultimate star-formation feedback factor in galaxies, able to oper
Expediency
发表于 2025-3-22 15:42:46
How to Reach a Point of No Return,o determine the cosmic-ray ionisation rate (especially the cosmic-ray spectrum at . < 1 GeV and the ionisation cross sections), and calculate the ionisation rate as a function of the column density of molecular hydrogen. Available data support the existence of a low-energy component (below ∼ 100 MeV
Expediency
发表于 2025-3-22 20:08:27
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CHOIR
发表于 2025-3-22 22:00:19
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澄清
发表于 2025-3-23 05:07:28
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pulmonary-edema
发表于 2025-3-23 05:44:26
Space as the Next Theater of War,. These processes drive the chemical pathways of formation of gas phase molecules which later can be adsorbed onto the surface of grains. We improve on previously existing chemical models by treating the interaction of cosmic rays with the gas/grain environment in a way that is consistent with the l