Source: The Astrophysical Journal. Unidade: IAG
Subjects: ACELERAÇÃO DE PARTÍCULAS, BURACOS NEGROS, RAIOS GAMA, RADIAÇÃO TÉRMICA, RADIAÇÃO NÃO TÉRMICA
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ABNT
GUIRIEC, S et al. Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation. The Astrophysical Journal, v. 807, p. 148/1-148/55, 2015Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/807/2/148. Acesso em: 30 abr. 2024.APA
Guiriec, S., Kouveliotou, C., Daigne, F., & Souza, R. N. da. (2015). Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation. The Astrophysical Journal, 807, 148/1-148/55. doi:10.1088/0004-637X/807/2/148NLM
Guiriec S, Kouveliotou C, Daigne F, Souza RN da. Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation [Internet]. The Astrophysical Journal. 2015 ; 807 148/1-148/55.[citado 2024 abr. 30 ] Available from: https://doi.org/10.1088/0004-637X/807/2/148Vancouver
Guiriec S, Kouveliotou C, Daigne F, Souza RN da. Toward a better understanding of the GRB phenomenon: a new model for GRB prompt emission and its effects on the new LiNT-- E rest.NT peak, i relation [Internet]. The Astrophysical Journal. 2015 ; 807 148/1-148/55.[citado 2024 abr. 30 ] Available from: https://doi.org/10.1088/0004-637X/807/2/148
