Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | García, Federico | - |
| dc.creator | Zhang, Guobao | - |
| dc.creator | Méndez, Mariano | - |
| dc.date | 2015-06-05T20:25:18Z | - |
| dc.date | 2015-06-05T20:25:18Z | - |
| dc.date | 2013-03 | - |
| dc.date | 2016-03-30 10:35:44.97925-03 | - |
| dc.date.accessioned | 2019-04-29T15:51:09Z | - |
| dc.date.available | 2019-04-29T15:51:09Z | - |
| dc.date.issued | 2013-03 | - |
| dc.identifier | García, Federico; Zhang, Guobao ; Méndez, Mariano; The cooling phase of Type I X-ray bursts observed with RXTE in 4U 1820-30 does not follow the canonical F-T^4 relation; Wiley-blackwell Publishing, Inc; Monthly Notices Of The Royal Astronomical Society; 429; 3-2013; 3266-3271; | - |
| dc.identifier | 0035-8711 | - |
| dc.identifier | http://hdl.handle.net/11336/618 | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/303728 | - |
| dc.description | We analysed the complete set of bursts from the neutron star low-mass X-ray binary 4U 1820-30 detected with the Rossi X-ray Timing Explorer (RXTE). We found that all are photospheric radius expansion bursts, and have similar duration, peak flux and fluence. From the analysis of time-resolved spectra during the cooling phase of the bursts, we found that the relation between the bolometric flux and the temperature is very different from the canonical F-T^4 relation which is expected if the apparent emitting area on the surface of the neutron star remains constant. The flux-temperature relation can be fitted using a broken power law, with indices v1 = 2.0 +/- 0.3 and v2 = 5.72 +/- 0.06. The departure from the F-T^4 relation during the cooling phase of the X-ray bursts in 4U 1820-30 could be due to changes in the emitting area of the neutron star while the atmosphere cools down, variations in the colour-correction factor due to chemical evolution, or the presence of a source of heat, e.g. residual hydrogen nuclear burning, playing an important role when the burst emission ceases. | - |
| dc.description | Fil: García, Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - La Plata. Instituto Argentino de Radioastronomia (i); Argentina; | - |
| dc.description | Fil: Zhang, Guobao. Kapteyn Astronomical Institute. University of Groningen; Holanda; | - |
| dc.description | Fil: Méndez, Mariano. Kapteyn Astronomical Institute. University of Groningen; Holanda; | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | Wiley-blackwell Publishing, Inc | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://mnras.oxfordjournals.org/content/429/4/3266 | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.subject | STARS: INDIVIDUAL: 4U 1820-30 | - |
| dc.subject | STARS: NEUTRON | - |
| dc.subject | X-RAYS: BINARIES | - |
| dc.subject | X-RAYS: BURSTS | - |
| dc.subject | Ciencias Naturales y Exactas | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | Astronomía (incluye Astrofísica y Ciencias del Espacio) | - |
| dc.title | The cooling phase of Type I X-ray bursts observed with RXTE in 4U 1820-30 does not follow the canonical F-T^4 relation | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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