Source:http://linkedlifedata.com/resource/pubmed/id/11062121
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rdf:type | |
lifeskim:mentions | |
pubmed:issue |
5493
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pubmed:dateCreated |
2000-11-7
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pubmed:abstractText |
We report on the discovery of two emission features observed in the x-ray spectrum of the afterglow of the gamma-ray burst (GRB) of 16 December 1999 by the Chandra X-ray Observatory. These features are identified with the Ly(alpha) line and the narrow recombination continuum by hydrogenic ions of iron at a redshift z = 1.00 +/- 0.02, providing an unambiguous measurement of the distance of a GRB. Line width and intensity imply that the progenitor of the GRB was a massive star system that ejected, before the GRB event, a quantity of iron approximately 0.01 of the mass of the sun at a velocity approximately 0.1 of the speed of light, probably by a supernova explosion.
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pubmed:language |
eng
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pubmed:journal | |
pubmed:status |
PubMed-not-MEDLINE
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pubmed:month |
Nov
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pubmed:issn |
0036-8075
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pubmed:author |
pubmed-author:BradtHH,
pubmed-author:CostaEE,
pubmed-author:FerociMM,
pubmed-author:FrailDD,
pubmed-author:FronteraFF,
pubmed-author:GarciaMM,
pubmed-author:GarmireGG,
pubmed-author:HalpernJJ,
pubmed-author:HeiseJJ,
pubmed-author:HurleyKK,
pubmed-author:KawaiNN,
pubmed-author:KippenR MRM,
pubmed-author:MészárosPP,
pubmed-author:MarshallFF,
pubmed-author:MurakamiTT,
pubmed-author:PiroLL,
pubmed-author:SokolovV VVV,
pubmed-author:StrattaGG,
pubmed-author:TakeshimaTT,
pubmed-author:VietriMM,
pubmed-author:YoshidaAA
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pubmed:issnType |
Print
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pubmed:day |
3
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pubmed:volume |
290
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pubmed:owner |
NLM
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pubmed:authorsComplete |
Y
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pubmed:pagination |
955-8
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pubmed:dateRevised |
2007-3-19
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pubmed:year |
2000
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pubmed:articleTitle |
Observation of X-ray lines from a gamma-ray burst (GRB991216): evidence of moving ejecta from the progenitor.
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pubmed:affiliation |
Istituto Astrofisica Spaziale, Consiglio Nazionale delle Ricerche (CNR), Via Fosso del Cavaliere, 00133 Roma, Italy. piro@ias.rm.cnr.it
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pubmed:publicationType |
Journal Article
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