LIN Yi-qing. The Lorentz Factor and Viewing Angle of GRB 170817A[J]. Acta Astronomica Sinica, 2020, 61(1): 6. DOI: 10.15940/j.cnki.0001-5245.2020.01.006
Citation:
LIN Yi-qing. The Lorentz Factor and Viewing Angle of GRB 170817A[J]. Acta Astronomica Sinica, 2020, 61(1): 6. DOI: 10.15940/j.cnki.0001-5245.2020.01.006
LIN Yi-qing. The Lorentz Factor and Viewing Angle of GRB 170817A[J]. Acta Astronomica Sinica, 2020, 61(1): 6. DOI: 10.15940/j.cnki.0001-5245.2020.01.006
Citation:
LIN Yi-qing. The Lorentz Factor and Viewing Angle of GRB 170817A[J]. Acta Astronomica Sinica, 2020, 61(1): 6. DOI: 10.15940/j.cnki.0001-5245.2020.01.006
The Lorentz Factor and Viewing Angle of GRB 170817A
Gamma-ray burst (GRB) 170817A, accompanied by the gravitational wave event GW170817, provides the first direct evidence for a link between a neutron star binary merger and a short duration GRB. GRB 170817A has an extremely weak luminosity, suggesting the jet may be off-axis to the line of sight. The relations between the peak energy E_p,i
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