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  • 1
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    GRB 090423 at a redshift of z approximately 8.1 (2009)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2009-10-30
    Description: Gamma-ray bursts (GRBs) are produced by rare types of massive stellar explosion. Their rapidly fading afterglows are often bright enough at optical wavelengths that they are detectable at cosmological distances. Hitherto, the highest known redshift for a GRB was z = 6.7 (ref. 1), for GRB 080913, and for a galaxy was z = 6.96 (ref. 2). Here we report observations of GRB 090423 and the near-infrared spectroscopic measurement of its redshift, z = 8.1(-0.3)(+0.1). This burst happened when the Universe was only about 4 per cent of its current age. Its properties are similar to those of GRBs observed at low/intermediate redshifts, suggesting that the mechanisms and progenitors that gave rise to this burst about 600,000,000 years after the Big Bang are not markedly different from those producing GRBs about 10,000,000,000 years later.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Salvaterra, R -- Valle, M Della -- Campana, S -- Chincarini, G -- Covino, S -- D'Avanzo, P -- Fernandez-Soto, A -- Guidorzi, C -- Mannucci, F -- Margutti, R -- Thone, C C -- Antonelli, L A -- Barthelmy, S D -- De Pasquale, M -- D'Elia, V -- Fiore, F -- Fugazza, D -- Hunt, L K -- Maiorano, E -- Marinoni, S -- Marshall, F E -- Molinari, E -- Nousek, J -- Pian, E -- Racusin, J L -- Stella, L -- Amati, L -- Andreuzzi, G -- Cusumano, G -- Fenimore, E E -- Ferrero, P -- Giommi, P -- Guetta, D -- Holland, S T -- Hurley, K -- Israel, G L -- Mao, J -- Markwardt, C B -- Masetti, N -- Pagani, C -- Palazzi, E -- Palmer, D M -- Piranomonte, S -- Tagliaferri, G -- Testa, V -- England -- Nature. 2009 Oct 29;461(7268):1258-60. doi: 10.1038/nature08445.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉INAF, Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate (LC), Italy. salvaterra@mib.infn.it〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/19865166" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
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  • 2
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    The unusual gamma-ray burst GRB 101225A explained as a minor body falling onto a neutron star (2011)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2011-12-02
    Description: The tidal disruption of a solar-mass star around a supermassive black hole has been extensively studied analytically and numerically. In these events, the star develops into an elongated banana-shaped structure. After completing an eccentric orbit, the bound debris falls into the black hole, forming an accretion disk and emitting radiation. The same process may occur on planetary scales if a minor body passes too close to its star. In the Solar System, comets fall directly into our Sun or onto planets. If the star is a compact object, the minor body can become tidally disrupted. Indeed, one of the first mechanisms invoked to produce strong gamma-ray emission involved accretion of comets onto neutron stars in our Galaxy. Here we report that the peculiarities of the 'Christmas' gamma-ray burst (GRB 101225A) can be explained by a tidal disruption event of a minor body around an isolated Galactic neutron star. This would indicate either that minor bodies can be captured by compact stellar remnants more frequently than occurs in the Solar System or that minor-body formation is relatively easy around millisecond radio pulsars. A peculiar supernova associated with a gamma-ray burst provides an alternative explanation.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Campana, S -- Lodato, G -- D'Avanzo, P -- Panagia, N -- Rossi, E M -- Della Valle, M -- Tagliaferri, G -- Antonelli, L A -- Covino, S -- Ghirlanda, G -- Ghisellini, G -- Melandri, A -- Pian, E -- Salvaterra, R -- Cusumano, G -- D'Elia, V -- Fugazza, D -- Palazzi, E -- Sbarufatti, B -- Vergani, S D -- England -- Nature. 2011 Nov 30;480(7375):69-71. doi: 10.1038/nature10592.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉INAF - Osservatorio Astronomico di Brera, Via E. Bianchi 46, I-23807 Merate, Italy. sergio.campana@brera.inaf.it〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22129725" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
    Location Call Number Expected Availability
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