我没有辱骂
发表于 2025-3-21 20:08:15
书目名称Gamma-Ray Bursts影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0380610<br><br> <br><br>书目名称Gamma-Ray Bursts读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0380610<br><br> <br><br>
意外
发表于 2025-3-21 22:51:48
The BATSE decade,ed to study GRBs. BATSE consisted of eight pairs of NaI detectors. Each pair included a Large Area Detector (LAD) and a Spectroscopy Detector (SD). The area of a Large Area Detector was 2000 cm.. With a sensitivity 5 to 10 times better than previous GRB detectors, BATSE detected an average of 1 GRB
表否定
发表于 2025-3-22 03:01:27
BeppoSAX and the afterglow era,bout the mission and its instruments. In the introduction to this chapter, it is important to mention the remarkable work done by the scientific and technical teams, which were strongly motivated by two researchers, E. Costa and F. Frontera. These two reseachers were very excited by the GRB mystery
nascent
发表于 2025-3-22 07:43:30
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Intuitive
发表于 2025-3-22 09:59:00
,Gamma-ray bursts—fireballs and blastwaves, the main properties of gamma-ray bursts with standard physics applied to somewhat ‘exotic’ objects. In this chapter we outline the most popular model to explain GRBs and their afterglows. This model, with its basic ingredients, has very often been called the standard model.
overwrought
发表于 2025-3-22 13:08:39
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overwrought
发表于 2025-3-22 17:49:59
Early afterglows: the Swift revolution,ontributed to a better knowledge of GRBs. In particular, these observations contributed to a better appreciation of the connection between the GRB prompt emission and the afterglow. Swift has brought various surprises: the complex behavior of the early X-ray afterglow (., .), the frequent faintness
TAP
发表于 2025-3-22 21:44:20
Progenitors,ts have made it possible to measure the isotropic equivalent energies emitted by GRBs in gamma-rays. These energies reach 10. to 10. erg. As most GRBs are probably collimated with typical opening angles between 1° and 20°, the true energy is clustered around 10. to 10. ergs which must be liberated i
精美食品
发表于 2025-3-23 02:59:14
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压倒性胜利
发表于 2025-3-23 08:35:38
https://doi.org/10.1007/978-3-540-39088-6Cosmology; Universe; astrophysics; gamma-ray bursts; stellar explosions; supernovae