Gamma-ray bursts /
As the most powerful explosion that occurs in the universe, gamma-ray bursts (GRBs) are one of the most exciting topics being studied in astrophysics. Creating more energy than the Sun does in its entire lifetime, GRBs create a blaze of light that will outshine every other object visible in the sky,...
Clasificación: | Libro Electrónico |
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Autor principal: | |
Formato: | Electrónico eBook |
Idioma: | Inglés |
Publicado: |
Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) :
IOP Publishing,
[2018]
|
Colección: | IOP (Series). Release 5.
AAS-IOP astronomy. Release 1. |
Temas: | |
Acceso en línea: | Texto completo |
MARC
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020 | |a 9780750315012 |q mobi | ||
020 | |z 9780750315005 |q print | ||
024 | 7 | |a 10.1088/2514-3433/aae164 |2 doi | |
035 | |a (CaBNVSL)thg00978446 | ||
035 | |a (OCoLC)1082881978 | ||
040 | |a CaBNVSL |b eng |e rda |c CaBNVSL |d CaBNVSL | ||
050 | 4 | |a QB471.7.B85 |b L484 2018eb | |
072 | 7 | |a PGM |2 bicssc | |
072 | 7 | |a SCI004000 |2 bisacsh | |
082 | 0 | 4 | |a 522/.6862 |2 23 |
100 | 1 | |a Levan, Andrew J., |e author. | |
245 | 1 | 0 | |a Gamma-ray bursts / |c Andrew Levan. |
264 | 1 | |a Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) : |b IOP Publishing, |c [2018] | |
300 | |a 1 online resource (various pagings) : |b illustrations (some color). | ||
336 | |a text |2 rdacontent | ||
337 | |a electronic |2 isbdmedia | ||
338 | |a online resource |2 rdacarrier | ||
490 | 1 | |a [IOP release 5] | |
490 | 1 | |a AAS-IOP astronomy. [release 1], |x 2514-3433 | |
500 | |a "Version: 20181201"--Title page verso. | ||
504 | |a Includes bibliographical references. | ||
505 | 0 | |a 1. A historical primer -- 1.1. A lesson in serendipity -- 1.2. GRB phenomenology -- 1.3. The early years -- 1.4. Suggested models for GRB creation -- 1.5. Intensive efforts and large samples -- 1.6. The fireball shock model -- 1.7. The long-GRB afterglow revolution -- 1.8. Redshifts and host galaxies -- 1.9. The supernova connection -- 1.10. GRB energetics -- 1.11. The Neil Gehrels Swift era -- 1.12. New insights from fermi -- 1.13. Multimessenger astronomy -- 1.14. Summary | |
505 | 8 | |a 2. Prompt emission -- 2.1. Observational properties -- 2.2. Origin of the prompt emission -- 2.3. Summary | |
505 | 8 | |a 3. Afterglow emission -- 3.1. The first afterglow searches -- 3.2. X-ray afterglows -- 3.3. Optical afterglows -- 3.4. Radio/submillimeter afterglows -- 3.5. Emission processes -- 3.6. Evidence for relativistic beaming | |
505 | 8 | |a 4. Central engines -- 4.1. The requirement of a central engine -- 4.2. Black hole central engines -- 4.3. Magnetar central engines -- 4.4. Central engines in other astrophysical transients -- 4.5. Summary | |
505 | 8 | |a 5. Long-GRB progenitors -- 5.1. The GRB-supernova connection -- 5.2. Observational constraints on stellar masses and sizes -- 5.3. Other populations of long-duration GRBs -- 5.4. Low-luminosity GRBs -- 5.5. Extremely long gamma-ray transients -- 5.6. Constraints for GRB production -- 5.7. Binary or single? | |
505 | 8 | |a 6. Short-GRB progenitors -- 6.1. Introduction -- 6.2. Progenitor models -- 6.3. Prompt emission properties -- 6.4. Afterglow properties -- 6.5. Host galaxy properties -- 6.6. Locations -- 6.7. Redshifts and energetics -- 6.8. Radioactively driven transients -- 6.9. Gravitational-wave emission | |
505 | 8 | |a 7. GRBs as cosmological probes -- 7.1. A range of cosmological probes -- 7.2. Science from high-z GRB afterglows -- 7.3. GRBs beyond z [tilde operator] 5 -- 7.4. GRBs from population iii stars -- 7.5. The universal star formation rate -- 7.6. Cosmological parameters from GRBs -- 7.7. The GRB hubble diagram | |
505 | 8 | |a 8. Long-GRB host galaxies -- 8.1. Early observations -- 8.2. GRB hosts in the galaxy zoo -- 8.3. Basic properties of long-GRB hosts -- 8.4. Building meaningful samples of GRB hosts -- 8.5. GRBs hosts at optical and ir wavelengths -- 8.6. GRB hosts at submillimeter and radio wavelengths -- 8.7. GRB hosts as tools to probe progenitors -- 8.8. GRB hosts as tools to probe distant galaxies -- 8.9. Burst locations and environments -- 8.10. Comparative properties of GRB hosts with other core-collapse events | |
505 | 8 | |a 9. Multimessenger astronomy -- 9.1. From multiwavelength to multimessenger astronomy -- 9.2. Gravitational waves -- 9.3. Sources of gravitational-wave emission -- 9.4. Gravitational-wave horizons -- 9.5. Prospect for joint detections -- 9.6. Electromagnetic searches in black hole-black hole mergers -- 9.7. GW 170817 and GRB 170817a -- 9.8. Gravitational wave-electromagnetic detections : questions for the future -- 9.9. Neutrino emission -- 9.10. Ultra-high-energy cosmic rays -- 9.11. Summary | |
505 | 8 | |a 10. GRB astronomy : summary and future outlook -- 10.1. Challenges for the future -- 10.2. Possibilities for future GRB detection missions -- 10.3. The crucial role of follow-up -- 10.4. Summary. | |
520 | 3 | |a As the most powerful explosion that occurs in the universe, gamma-ray bursts (GRBs) are one of the most exciting topics being studied in astrophysics. Creating more energy than the Sun does in its entire lifetime, GRBs create a blaze of light that will outshine every other object visible in the sky, enabling us to measure galaxies that are several million years old. | |
530 | |a Also available in print. | ||
538 | |a Mode of access: World Wide Web. | ||
538 | |a System requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader. | ||
545 | |a Andrew Levan is a professor of astronomy and astrophysics at The University of Warwick. He has spent most of his career focussing on the origins of gamma-ray bursts and their use as cosmic probes, utilising a wide range of ground- and space-based telescopes across the electromagnetic spectrum. | ||
588 | 0 | |a Title from PDF title page (viewed on January 16, 2019). | |
650 | 0 | |a Gamma ray bursts. | |
650 | 7 | |a Galaxies & stars. |2 bicssc | |
650 | 7 | |a SCIENCE / Astronomy. |2 bisacsh | |
710 | 2 | |a Institute of Physics (Great Britain), |e publisher. | |
776 | 0 | 8 | |i Print version: |z 9780750315005 |
830 | 0 | |a IOP (Series). |p Release 5. | |
830 | 0 | |a AAS-IOP astronomy. |p Release 1. | |
856 | 4 | 0 | |u https://iopscience.uam.elogim.com/book/978-0-7503-1502-9 |z Texto completo |