Gamma Ray Bursts in the Afterglow Era

By Federico Frontera. 2003

324 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/6c168ffc2e668eae512694ba48aeee54ea868ed7

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In Astronomy and Astrophysics

1. Bing Zhang
2. Stan Woosley
3. N. Langer
4. A. Ferrara
5. P. Mészáros
6. A. Pe’er
7. N. Gehrels
8. E. Berger

Citations in the corpus

• Efficient acceleration and radiation in Poynting flux powered GRB outflows (2002, unknown): “We speculated in Paper II about the possibility that these low-(cid:27) 0 outflows could be identified with X-ray flashes observed by BeppoSAX (Heise et al. 2001; Heise & in ’t Zand 2002).”
• Acceleration of GRB outflows by Poynting flux dissipation (2001, background): “2001, hereafter Paper I). Secondly, it leads to an outward decrease of magnetic pressure, which causes a strong acceleration of the flow and conversion of Poynting flux to kinetic energy. In the present work, we concentrate on the acceleration effect, and show how it depends on the parameters (energ”
• INTEGRAL observations of recurrent fast X-ray transient sources (2005, unknown): “6−1703 – X-rays: general – X-rays: individuals: XTE J1739−302/IGR J17391−302 – X-rays: binaries – gamma rays: observations”
• SPI: The spectrometer aboard INTEGRAL (2003, background): “The ACS provides a large eff ctive area for the detection of bursts (von Kienlin et al. 2003; von Kienlin et al. 2001; Hurley 1997; Lichti et al. 2000), but unfortunately with no (or only very coarse) positional information.”
• The Propagation and Eruption of Relativistic Jets from the Stellar Progenitors of Gamma-Ray Bursts (2003, methodology): “Subject headings: gamma rays: bursts — hydrodynamics — methods: numerical — relativity”
• The Observable Effects of a Photospheric Component on GRB and XRF Prompt Emission Spectrum (2005, background): “This peak energy is consistent with the peak energy observed in X-ray flashes at ∼ 25 keV (Heise et al. 2001) and X-ray-rich GRB’s (XRR’s), which show peak energy clustering at ∼ 50 keV (Sakamoto et al. 2005).”
• On the Collapsar Model of Long Gamma-Ray Bursts:Constraints from Cosmic Metallicity Evolution (2005, methodology): “1; see also Firmani et al. (2005) • Local massive galaxies, like our Milkyway, are not expected to host long GRBs.”
• Discovery of the short γ-ray burst GRB 050709 (2005, result): “and its spectrum is much harder than these were for GRB 020531, the other short-hard burst localized by HETE.(15) We also note that the time history and the spectral properties of GRB 050709 are similar to those of several Burst and Transient Source Experiment (BATSE) bursts, including GRBs 921022, ”