Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/28015
Campo DC | Valore | Lingua |
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dc.contributor.author | Court, J. M. C. | en_US |
dc.contributor.author | Altamirano, D. | en_US |
dc.contributor.author | Albayati, A. C. | en_US |
dc.contributor.author | SANNA, ALBERTO | en_US |
dc.contributor.author | BELLONI, Tomaso Maria Melchiorre | en_US |
dc.contributor.author | Overton, T. | en_US |
dc.contributor.author | Degenaar, N. | en_US |
dc.contributor.author | Wijnands, R. | en_US |
dc.contributor.author | Yamaoka, K. | en_US |
dc.contributor.author | Hill, A. B. | en_US |
dc.contributor.author | Knigge, C. | en_US |
dc.date.accessioned | 2020-10-27T10:05:44Z | - |
dc.date.available | 2020-10-27T10:05:44Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28015 | - |
dc.description.abstract | GRO J1744-28, commonly known as the `Bursting Pulsar', is a low-mass X-ray binary containing a neutron star and an evolved giant star. This system, together with the Rapid Burster (MXB 1730-33), are the only two systems that display the so-called type II X-ray bursts. These types of bursts, which last for tens of seconds, are thought to be caused by viscous instabilities in the disc; however, the type II bursts seen in GRO J1744-28 are qualitatively very different from those seen in the archetypal type II bursting source, the Rapid Burster. To understand these differences and to create a framework for future study, we perform a study of all X-ray observations of all three known outbursts of the Bursting Pulsar which contained type II bursts, including a population study of all type II X-ray bursts seen by RXTE. We find that the bursts from this source are best described in four distinct phenomena or `classes' and that the characteristics of the bursts evolve in a predictable way. We compare our results with what is known for the Rapid Burster and put out results in the context of models that try to explain this phenomena. | en_US |
dc.language.iso | eng | en_US |
dc.title | The evolution of X-ray bursts in the `Bursting Pulsar' GRO J1744-28 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/sty2312 | en_US |
dc.identifier.scopus | 2-s2.0-85060881762 | en_US |
dc.identifier.isi | 000449764000060 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/481/2/2273/5086081 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 481 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2273 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2018MNRAS.481.2273C | 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.cerifentitytype | Publications | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0001-9621-3796 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
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court.pdf | Pdf editoriale | 9.98 MB | Adobe PDF | Visualizza/apri |
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