The cooling phase of Type I X-ray bursts observed with RXTE in 4U 1820-30 does not follow the canonical F \ensuremath∝ T$^{4}$ relation. Garcı́a, Federico, Zhang, G., & Méndez, M. \mnras, 429(4):3266-3271, March, 2013.
doi  bibtex   
@ARTICLE{2013MNRAS.429.3266G,
       author = {{Garc{\'\i}a}, Federico and {Zhang}, Guobao and {M{\'e}ndez}, Mariano},
        title = "{The cooling phase of Type I X-ray bursts observed with RXTE in 4U 1820-30 does not follow the canonical F {\ensuremath{\propto}} T$^{4}$ relation}",
      journal = {\mnras},
     keywords = {stars: individual: 4U 1820-30, stars: neutron, X-rays: binaries, X-rays: bursts, Astrophysics - High Energy Astrophysical Phenomena},
         year = 2013,
        month = mar,
       volume = {429},
       number = {4},
        pages = {3266-3271},
          doi = {10.1093/mnras/sts583},
archivePrefix = {arXiv},
       eprint = {1301.1035},
 primaryClass = {astro-ph.HE},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2013MNRAS.429.3266G},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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