Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27936
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Cerda-Duran, Pablo | en_US |
dc.contributor.author | ELIAS DE LA ROSA, NANCY DEL CARMEN | en_US |
dc.date.accessioned | 2020-10-22T15:52:25Z | - |
dc.date.available | 2020-10-22T15:52:25Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.isbn | 978-3-319-97615-0 | en_US |
dc.identifier.isbn | 978-3-319-97616-7 | en_US |
dc.identifier.issn | 0067-0057 | en |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27936 | - |
dc.description.abstract | In the last decade there has been a remarkable increase in our knowledge about core-collapse supernovae (CC-SNe), and the birthplace of neutron stars, from both the observational and the theoretical point of view. Since the 1930s, with the first systematic supernova search, the techniques for discovering and studying extragalactic SNe have improved. Many SNe have been observed, and some of them, have been followed through efficiently and with detail. Furthermore, there has been a significant progress in the theoretical modelling of the scenario, boosted by the arrival of new generations of supercomputers that have allowed to perform multidimensional numerical simulations with unprecedented detail and realism. The joint work of observational and theoretical studies of individual SNe over the whole range of the electromagnetic spectrum has allowed to derive physical parameters, which constrain the nature of the progenitor, and the composition and structure of the star's envelope at the time of the explosion. The observed properties of a CC-SN are an imprint of the physical parameters of the explosion such as mass of the ejecta, kinetic energy of the explosion, the mass loss rate, or the structure of the star before the explosion. In this chapter, we review the current status of SNe observations and theoretical modelling, the connection with their progenitor stars, and the properties of the neutron stars left behind. | en_US |
dc.language.iso | eng | en_US |
dc.title | Neutron Stars Formation and Core Collapse Supernovae | en_US |
dc.type | Book part | - |
dc.identifier.doi | 10.1007/978-3-319-97616-7_1 | en_US |
dc.identifier.url | https://link.springer.com/chapter/10.1007%2F978-3-319-97616-7_1 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 457 | en_US |
dc.relation.firstpage | 1 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 2 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | ESP | en_US |
dc.relation.allauthors | Rezzolla, Luciano; Pizzochero, Pierre; Jones, David Ian; Rea, Nanda; Vidaña, Isaac | en_US |
dc.relation.ispartofbook | The Physics and Astrophysics of Neutron Stars | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 268 Contributo in volume (Capitolo o Saggio) | - |
dc.relation.series | ASTROPHYSICS AND SPACE SCIENCE LIBRARY | en_US |
dc.identifier.adsbibcode | 2018ASSL..457....1C | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Book part | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | reserved | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0002-1381-9125 | - |
crisitem.journal.journalissn | 0067-0057 | - |
crisitem.journal.ance | E016260 | - |
Appears in Collections: | 2.01 Capitoli o saggi in libro |
Files in This Item:
File | Description | Size | Format | Existing users please |
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Cerdan_2018ASSL..457....1C_preprint.pdf | postprint | 908.88 kB | Adobe PDF | |
Chapter_NeutronStarsFormationAndCoreCo.pdf | [Administrators only] | 1.72 MB | Adobe PDF |
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