SCOWL
发表于 2025-3-21 18:13:10
书目名称Astrophysical Sources of High Energy Particles and Radiation影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0163685<br><br> <br><br>书目名称Astrophysical Sources of High Energy Particles and Radiation读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0163685<br><br> <br><br>
A精确的
发表于 2025-3-21 21:07:19
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hallow
发表于 2025-3-22 02:55:34
https://doi.org/10.1007/978-1-4302-0103-8nduced γ-ray flux from SNR at least on an order of magnitude, that allows to adjust the theoretical π° decay γ-luminosities with observed fluxes at least for a few SNRs even for low density (no ~ 10. -4- 10. cm.) cloud.
Crumple
发表于 2025-3-22 06:55:27
https://doi.org/10.1007/978-1-4302-0103-8the characteristic decay time, ..: ~ 10. ≥ .. > 10. yrs, can be excluded assuming the standard initial magnetic momentum, μo =10.Gcm., if accreting INSs are observed. For these parameters an INS would never reach the stage of accretion from the interstellar medium even for a low space velocity of th
Type-1-Diabetes
发表于 2025-3-22 09:19:30
Forward Kinematics: Making Things Walkthe direction, the source could be identified and the afterglow of the burst at these longer wavelengths could be observed continuously, upto several weeks after the burst. Detailed measurements in the 7-ray window were made with the BATSE instrument aboard the . — we will review these before descri
CHAR
发表于 2025-3-22 14:55:35
Forward Kinematics: Making Things Walks of solar FEP (especially in periods of very great events) . 3.- by properties of solar FEP interaction with solar wind matter accompanied with GR generation through decay of neutral pions .
RACE
发表于 2025-3-22 19:36:52
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Complement
发表于 2025-3-22 23:42:14
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浓缩
发表于 2025-3-23 01:47:21
Dark Matter Halo of Our Galaxy cluster has to be in some unseen form to account for the large observed value of the velocity dispersion. This work was followed up by a few other workers and finally in 1972 based on observations of the velocities of hundreds of galaxies in the cluster, Rood et al., confirmed that atleast 75 %
BOOST
发表于 2025-3-23 09:12:11
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