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At peak, long-duration gamma-ray bursts are the most luminous sources of electromagnetic radiation known. Since their progenitors are massive stars, they provide a tracer of star formation and star-forming galaxies over the whole of cosmic history. Their bright power-law afterglows provide ideal bac...

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Veröffentlicht in:	Exper.Astron 2021-12, Vol.52 (3), p.219-244
Hauptverfasser:	Tanvir, N. R., Le Floc’h, E., Christensen, L., Caruana, J., Salvaterra, R., Ghirlanda, G., Ciardi, B., Maio, U., D’Odorico, V., Piedipalumbo, E., Campana, S., Noterdaeme, P., Graziani, L., Amati, L., Bagoly, Z., Balázs, L. G., Basa, S., Behar, E., De Cia, A., Valle, M. Della, De Pasquale, M., Frontera, F., Gomboc, A., Götz, D., Horvath, I., Hudec, R., Mereghetti, S., O’Brien, P. T., Osborne, J. P., Paltani, S., Rosati, P., Sergijenko, O., Stanway, E. R., Szécsi, D., Tot́h, L. V., Urata, Y., Vergani, S., Zane, S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Afterglows Astronomy Astronomy & Astrophysics Backlights Chemistry and Earth Sciences Computer Science Dark energy Electromagnetic radiation Equations of state Explosions Galactic evolution Gamma ray bursts Instrumentation and Detectors Intergalactic media Interstellar matter Ionization Luminosity Massive stars Observations and Techniques Original Article Physical Sciences Physics Physics and Astronomy Population III stars Red shift Science & Technology Star & galaxy formation Star formation rate Statistics for Engineering
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