The Explosion Mechanism of Core-Collapse Supernovae and Its Observational Signatures

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F20%3A10424636" target="_blank" >RIV/00216208:11320/20:10424636 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1007/978-3-030-38509-5_7" target="_blank" >https://doi.org/10.1007/978-3-030-38509-5_7</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1007/978-3-030-38509-5_7" target="_blank" >10.1007/978-3-030-38509-5_7</a>

Jazyk výsledku

angličtina

Název v původním jazyce

The Explosion Mechanism of Core-Collapse Supernovae and Its Observational Signatures

Popis výsledku v původním jazyce

The death of massive stars is shrouded in many mysteries. One of them is the mechanism that overturns the collapse of the degenerate iron core into an explosion, a process that determines the supernova explosion energy, properties of the surviving compact remnant, and the nucleosynthetic yields. The number of core-collapse supernova observations has been growing with an accelerating pace thanks to modern time-domain astronomical surveys and new tests of the explosion mechanism are becoming possible. We review predictions of parameterized supernova explosion models and compare them with explosion properties inferred from observed light curves, spectra, and neutron star masses.

Název v anglickém jazyce

The Explosion Mechanism of Core-Collapse Supernovae and Its Observational Signatures

Popis výsledku anglicky

The death of massive stars is shrouded in many mysteries. One of them is the mechanism that overturns the collapse of the degenerate iron core into an explosion, a process that determines the supernova explosion energy, properties of the surviving compact remnant, and the nucleosynthetic yields. The number of core-collapse supernova observations has been growing with an accelerating pace thanks to modern time-domain astronomical surveys and new tests of the explosion mechanism are becoming possible. We review predictions of parameterized supernova explosion models and compare them with explosion properties inferred from observed light curves, spectra, and neutron star masses.

Druh

C - Kapitola v odborné knize

CEP obor

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OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/LTAUSA18093" target="_blank" >LTAUSA18093: Časová proměnnost v astronomii: účast v projektu All-Sky Automated Survey for Supernovae</a><br>

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2020

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název knihy nebo sborníku

Reviews in Frontiers of Modern Astrophysic: From Space Debris to Cosmology

ISBN

978-3-030-38508-8

Počet stran výsledku

23

Strana od-do

189-211

Počet stran knihy

411

Název nakladatele

Springer

Místo vydání

Cham

Kód UT WoS kapitoly

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