脸红
发表于 2025-3-21 17:23:59
书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae影响因子(影响力)<br> http://impactfactor.cn/if/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae影响因子(影响力)学科排名<br> http://impactfactor.cn/ifr/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae网络公开度<br> http://impactfactor.cn/at/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae网络公开度学科排名<br> http://impactfactor.cn/atr/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae被引频次<br> http://impactfactor.cn/tc/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae被引频次学科排名<br> http://impactfactor.cn/tcr/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae年度引用<br> http://impactfactor.cn/ii/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae年度引用学科排名<br> http://impactfactor.cn/iir/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae读者反馈<br> http://impactfactor.cn/5y/?ISSN=BK0829362<br><br> <br><br>书目名称Revealing the Most Energetic Light from Pulsars and Their Nebulae读者反馈学科排名<br> http://impactfactor.cn/5yr/?ISSN=BK0829362<br><br> <br><br>
债务
发表于 2025-3-21 21:50:52
Pulsars and Pulsar Wind Nebulaesudden stop of the free-fall collapse leads to a rebound of the infalling matter triggering an outward shock that blows up the star envelope and powers a . supernova. If the mass of the progenitor star does not exceed .20 solar masses [.], the compact remnant core evolves into a .. Otherwise the amo
Amylase
发表于 2025-3-22 04:19:06
http://reply.papertrans.cn/83/8294/829362/829362_3.png
异端邪说2
发表于 2025-3-22 07:29:20
http://reply.papertrans.cn/83/8294/829362/829362_4.png
Armory
发表于 2025-3-22 11:54:53
Does PSR J0631 Power a Pulsar Wind Nebula?ost half of the current TeV .e population [.]. To increase the population with members situated in the outer part of our galaxy, . selected and observed 6 young and energetic gamma-ray pulsars that could potentially power TeV pulsar wind nebulae [.].
relieve
发表于 2025-3-22 13:27:31
http://reply.papertrans.cn/83/8294/829362/829362_6.png
子女
发表于 2025-3-22 19:04:19
MAGIC and the Crab Pulsar: History and Motivationpulsar). However, a significant portion of this 14% was taken as technical data to evaluate the performance of the instrument as described in Sect. ., and had no immediate scientific purpose. A short summary of the scientific observational campaigns on the Crab is given in Chap. ..
支架
发表于 2025-3-22 23:40:59
2190-5053from pulsars, together with a detailed compilation of VHE oThis book reports on the extraordinary observation of TeV gamma rays from the Crab Pulsar, the most energetic light ever detected from this type of object. It presents detailed information on the painstaking analysis of the unprecedentedly
贪心
发表于 2025-3-23 02:30:52
http://reply.papertrans.cn/83/8294/829362/829362_9.png
浮雕
发表于 2025-3-23 07:54:15
An Introduction to Very-High-Energy Astrophysicsere as illustrated by Fig. .. While for the visible and the radio part of the spectrum the atmosphere is mostly transparent, X-rays and gamma rays are completely absorbed by it. Only at the highest energy end, above a few tens of GeV, observing the violent absorption process in the atmosphere makes