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The bright optical afterglow of the long GRB 001007
J. M. Castro Cerón, A. J. Castro-Tirado, J. Gorosabel +35
We present optical follow up observations of the long GRB 001007 between 6.14 hours and ~468 days after the event. An unusually bright optical afterglow (OA) was seen to decline fo…
Diffuse gamma-ray line emission from multiple OB Associations in Cygnus
S. Plueschke, M. Cervino, R. Diehl +3
The COMPTEL observations of the diffuse galactic 1.809 MeV emission attributed to the radioactive decay of 26Al have confirmed the diffuse nature of this interstellar emission line…
Afterglow upper limits for four short duration, hard spectrum gamma-ray bursts
K. Hurley, E. Berger, A. Castro-Tirado +21
We present interplanetary network localization, spectral, and time history information for four short-duration, hard spectrum gamma-ray bursts, GRB000607, 001025B, 001204, and 0101…
Gamma-Ray Line Emission from Superbubbles in the Interstellar Medium: The Cygnus Region
S. Plueschke, R. Diehl, K. Kretschmer +2
The star forming process in the Milky Way is non-uniform in time and space. The scale of star forming regions ranges from groups within a few pc to large segments of spiral arms wi…
The Cygnus Region: 26Al from OB Associations
S. Plueschke, K. Kretschmer, R. Diehl +2
The COMPTEL map of the 1.809 MeV gamma-ray line, which is attributed to the radioactive decay of 26Al, shows significant excess emission in the Cygnus region. Cygnus is a region of…