Optical observations of GRB 060218/SN 2006aj and its host galaxy

Bibcode
2007AIPC..924..120F
DOI
10.1063/1.2774848
Ferrero, Patrizia; Palazzi, Eliana; Pian, Elena; Savaglio, Sandra
Referencia bibliográfica

THE MULTICOLORED LANDSCAPE OF COMPACT OBJECTS AND THEIR EXPLOSIVE ORIGINS. AIP Conference Proceedings, Volume 924, pp. 120-125 (2007).

Fecha de publicación:
8
2007
Número de autores
4
Número de autores del IAC
0
Número de citas
5
Número de citas referidas
4
Descripción
The supernova SN 2006aj associated with GRB 060218 is the second-closest GRB-SN observed to date (z=0.033) and is the clearest example of a SN associated with a Swift GRB with the earliest optical spectroscopy. Its optical data showed that this is the fastest evolving and among the least luminous GRB-SNe (70% as luminous as SN1998bw). However, its expansion velocity and a comparison with other stripped-envelope SNe suggest that SN2006aj is an intermediate object between Type Ic GRB-SNe and those not accompained by a GRB. High-resolution optical spectroscopy together with SDSS pre-burst observations revealed that the host galaxy of SN2006aj is a low-luminosity, metal-poor star-forming dwarf galaxy.
Tipo
Sin árbitro
Fuentes de rayos gamma
Estallidos de rayos gamma
Supernovas

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