The origin of the GRB diversity in the internal shock model

F. Daigne; R. Mochkovitch

doi:10.1393/ncb/i2007-10280-3

The origin of the GRB diversity in the internal shock model

F. Daigne
, R. Mochkovitch

Institut d’Astrophysique de Paris

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

Our knowledge of the GRB population has dramatically increased in the recent years. In addition to the "standard" bright cosmological GRBs observed by BATSE, Beppo-SAX and HETE2 have detected X-ray-rich GRBs, X-ray flashes, subenergetic GRBs and even a few "local" events (such as GRB 980425/SN1998bw). We describe how the internal shock model allows the existence of such a diversity in the GRB population.

langue originale	Anglais
Pages (de - à)	1465-1466
Nombre de pages	2
journal	Nuovo Cimento della Societa Italiana di Fisica B
Volume	121
Numéro de publication	12
Les DOIs	https://doi.org/10.1393/ncb/i2007-10280-3
état	Publié - 1 déc. 2006
Modification externe	Oui

Accès au document

10.1393/ncb/i2007-10280-3

Autres fichiers et liens

Lien vers la publication dans Scopus

Contient cette citation

@article{5cdc49ea405949c5bb655d6d2e1df8b7,

title = "The origin of the GRB diversity in the internal shock model",

abstract = "Our knowledge of the GRB population has dramatically increased in the recent years. In addition to the {"}standard{"} bright cosmological GRBs observed by BATSE, Beppo-SAX and HETE2 have detected X-ray-rich GRBs, X-ray flashes, subenergetic GRBs and even a few {"}local{"} events (such as GRB 980425/SN1998bw). We describe how the internal shock model allows the existence of such a diversity in the GRB population.",

author = "F. Daigne and R. Mochkovitch",

year = "2006",

month = dec,

day = "1",

doi = "10.1393/ncb/i2007-10280-3",

language = "English",

volume = "121",

pages = "1465--1466",

journal = "Nuovo Cimento della Societa Italiana di Fisica B",

issn = "1594-9982",

number = "12",

}

TY - JOUR

T1 - The origin of the GRB diversity in the internal shock model

AU - Daigne, F.

AU - Mochkovitch, R.

PY - 2006/12/1

Y1 - 2006/12/1

N2 - Our knowledge of the GRB population has dramatically increased in the recent years. In addition to the "standard" bright cosmological GRBs observed by BATSE, Beppo-SAX and HETE2 have detected X-ray-rich GRBs, X-ray flashes, subenergetic GRBs and even a few "local" events (such as GRB 980425/SN1998bw). We describe how the internal shock model allows the existence of such a diversity in the GRB population.

AB - Our knowledge of the GRB population has dramatically increased in the recent years. In addition to the "standard" bright cosmological GRBs observed by BATSE, Beppo-SAX and HETE2 have detected X-ray-rich GRBs, X-ray flashes, subenergetic GRBs and even a few "local" events (such as GRB 980425/SN1998bw). We describe how the internal shock model allows the existence of such a diversity in the GRB population.

UR - https://www.scopus.com/pages/publications/35348957909

U2 - 10.1393/ncb/i2007-10280-3

DO - 10.1393/ncb/i2007-10280-3

M3 - Article

AN - SCOPUS:35348957909

SN - 1594-9982

VL - 121

SP - 1465

EP - 1466

JO - Nuovo Cimento della Societa Italiana di Fisica B

JF - Nuovo Cimento della Societa Italiana di Fisica B

IS - 12

ER -

The origin of the GRB diversity in the internal shock model

Résumé

Accès au document

Autres fichiers et liens

Empreinte digitale

Contient cette citation