Constraining the mass of the GRB 030329 progenitor




Ostlin G, Zackrisson E, Sollerman J, Mattila S, Hayes M

PublisherWILEY-BLACKWELL

2008

Monthly Notices of the Royal Astronomical Society

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

MON NOT R ASTRON SOC

387

3

1227

1236

10

0035-8711

DOIhttps://doi.org/10.1111/j.1365-2966.2008.13319.x



These age estimates are an order of magnitude lower than the ages inferred from the overall host galaxy colours, indicating that progenitor mass estimates based on data for spatially unresolved GRB host galaxies will in general be of limited use. Our results are consistent with the collapsar scenario.



Last updated on 2025-14-10 at 10:09