Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/24432
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Beri, Aru | en_US |
dc.contributor.author | Paul, Biswajit | en_US |
dc.contributor.author | ORLANDINI, MAURO | en_US |
dc.contributor.author | Maitra, Chandreyee | en_US |
dc.date.accessioned | 2020-05-04T13:05:47Z | - |
dc.date.available | 2020-05-04T13:05:47Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 1384-1076 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/24432 | - |
dc.description.abstract | We have carried out a study of temperature evolution during thermonuclear bursts in LMXBs using broad band data from two instruments onboard BeppoSAX, the MECSand the PDS. However, instead of applying the standard technique of time resolved spectroscopy, we have determined the temperature in small time intervals using the ratio of count rates in the two instruments assuming a blackbody nature of burst emission and different interstellar absorption for different sources. Data from a total of twelve observations of six sources were analyzed during which 22 bursts were detected. We have obtained temperatures as high as ∼3.0 keV, even when there is no evidence of photospheric radius expansion. These high temperatures were observed in the sources within different broadband spectral states (soft and hard). | en_US |
dc.language.iso | eng | en_US |
dc.title | Temperature measurement during thermonuclear X-ray bursts with BeppoSAX | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1016/j.newast.2015.10.013 | en_US |
dc.identifier.scopus | 2-s2.0-84948395735 | en_US |
dc.identifier.isi | 000369200700008 | en_US |
dc.identifier.url | https://www.sciencedirect.com/science/article/abs/pii/S1384107615001335 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 45 | en_US |
dc.relation.issue | May 2016 | en_US |
dc.relation.firstpage | 48 | en_US |
dc.relation.lastpage | 53 | en_US |
dc.relation.numberofpages | 6 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | IND | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | NEW ASTRONOMY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016NewA...45...48B | en_US |
dc.relation.ercsector | Scienze Fisiche Settori ERC (ERC) di riferimento::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_10 High energy and particle astronomy – X-rays, cosmic rays, gamma rays, neutrinos | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegherò 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 | 1384-1076 | - |
crisitem.journal.ance | E117453 | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-0946-3151 | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
1510.04848.pdf | postprint | 704.79 kB | Adobe PDF | Visualizza/apri |
2016NewAst.45...48.pdf | [administrators only] | 483.14 kB | Adobe PDF |
Page view(s)
69
controllato il 18-lug-2024
Download(s)
22
controllato il 18-lug-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.