EDP Sciences 1776970373 20260423 fre

laboutique.edpsciences.fr-R000789 03 01 01 R000789 00 ED E107 00 01 01 Gamma-ray Bursts: 15 Years of GRB Afterglows Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe 01 eng 01 eng 08 701 03 22 99959928 17 16 00 06 01 https://laboutique.edpsciences.fr/flip_book/show/769 01 P1 EDP Sciences 01 01 P1 EDP Sciences 17 avenue du Hoggar - PA de Courtaboeuf - 91944 Les Ulis cedex A http://publications.edpsciences.org/ 02 01 001177 03 9782759810024 15 9782759810024 03 01 D1 EDP Sciences 29 https://laboutique.edpsciences.fr/open_access_download/1177/789 45 03 laboutique.edpsciences.fr-001177 03 01 01 001177 03 9782759810024 15 9782759810024 10 EA E107 10 00 01 R000789 ED E107 1 10 01 02 EAS Publication Series 01 01 Gamma-ray Bursts: 15 Years of GRB Afterglows Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe 1 B26 01 A1324 A.J. Castro-Tirado Castro-Tirado, A.J. A.J. Castro-Tirado 2 B26 01 A1325 J. Gorosabel Gorosabel, J. J. Gorosabel 3 B26 01 A1326 I.H. Park Park, I.H. I.H. Park 1 01 eng 01 eng 08 675 03 01 24 Izibook:Subject Astronomie 24 Izibook:Subject Astrophysique 24 Izibook:SubjectAndCategoryAndTags |Astronomie| 24 Izibook:SubjectAndCategoryAndTags |Astrophysique| 10 2011 SCI004000 10 2011 SCI005000 29 3066 01 520 06 05 00 <p>Gamma-ray bursts (GRB) are amongst the most energetic phenomena in the Universe. In 1997 (more than 15 years ago), BeppoSAX allowed the detection of the first GRB X-ray afterglow, leading to the detection of afterglows at other wavelengths (optical, radio) in the following years, probing the cosmological distance scale. There are still many other open issues which still need to be addressed, regarding both theoretical and observational aspects: prompt emission and afterglow physics, progenitors (including Pop III stars), host galaxies, multi-messenger information, etc.</p> 03 00 <p>Gamma-ray bursts (GRB) are amongst the most energetic phenomena in the Universe. In 1997 (more than 15 years ago), BeppoSAX allowed the detection of the first GRB X-ray afterglow, leading to the detection of afterglows at other wavelengths (optical, radio) in the following years, probing the cosmological distance scale. There are still many other open issues which still need to be addressed, regarding both theoretical and observational aspects: prompt emission and afterglow physics, progenitors (including Pop III stars), host galaxies, multi-messenger information, etc.</p> 02 00 Gamma-ray bursts (GRB) are amongst the most energetic phenomena in the Universe. In 1997 (more than 15 years ago), BeppoSAX allowed the detection of the first GRB X-ray afterglow, leading to the detection of afterglows at other wavelengths (optical, radio) in the following years, probing the cosmological distance scale. There are still many othe... 21 00 06 01 https://laboutique.edpsciences.fr/produit/734/9782759810024/gamma-ray-bursts-15-years-of-grb-afterglows 01 00 03 02 https://laboutique.edpsciences.fr/system/product_pictures/data/009/981/983/original/Gamma-ray_Bursts_eas61_cover.jpg 17 14 20240913T172448+0200 16 00 04 01 https://laboutique.edpsciences.fr/produit/734/9782759810024/gamma-ray-bursts-15-years-of-grb-afterglows/preview?escape=false#lg=1&slide=0 01 P1 EDP Sciences 01 01 P1 EDP Sciences 17 avenue du Hoggar - PA de Courtaboeuf - 91944 Les Ulis cedex A http://publications.edpsciences.org/ 04 01 00 20130712 19 00 20130712 2026 06 3052868830012 01 WORLD WORLD 08 EDP Sciences 04 01 00 20130712 03 01 D1 EDP Sciences 20 04 05 01 02 1 00 01 EUR