The cooling phase of Type I X-ray bursts observed with RXTE in 4U 1820−30 does not follow the canonical F ∝ T⁴ relation

We analysed the complete set of bursts from the neutron star low-mass X-ray binary 4U 1820-30 detected with the <i>ossi X-ray Timing Explorer</i> (<i> RXTE</i>). We found that all are photospheric radius expansion bursts, and have similar duration, peak flux and fluence. From...

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Detalles Bibliográficos
Autores principales: García, Federico, Zhang, Guobao, Méndez, Mariano R.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2013
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/127272
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