Titlebook: Gamma-Ray Bursts; The brightest explos Gilbert Vedrenne,Jean-Luc Atteia Book 2009 Springer-Verlag Berlin Heidelberg 2009 Cosmology.Universe

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書(shū)目名稱(chēng)Gamma-Ray Bursts影響因子(影響力)

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書(shū)目名稱(chēng)Gamma-Ray Bursts網(wǎng)絡(luò)公開(kāi)度

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書(shū)目名稱(chēng)Gamma-Ray Bursts被引頻次

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書(shū)目名稱(chēng)Gamma-Ray Bursts讀者反饋

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只看該作者 · 發(fā)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

只看該作者 · 發(fā)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

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只看該作者 · 發(fā)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.

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只看該作者 · 發(fā)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

只看該作者 · 發(fā)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

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只看該作者 · 發(fā)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

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