Astronomy and Astrophysics – Astrophysics
12 pages and 2 color figures, accepted for publication in Astrophysical Journal Letters
We apply a statistical method to derive very precise locations for soft gamma repeaters using data from the interplanetary network. We demonstrate the validity of the method by deriving a 600 arcsec^2 error ellipse for SGR1900+14 whose center agrees well with the VLA source position. We then apply it to SGR1806-20, for which we obtain a 230 arcsec^2 error ellipse, the smallest burst error box to date. We find that the most likely position of the source has a small but significant displacement from that of the non-thermal core of the radio supernova remnant G10.0-0.3, which was previously thought to be the position of the repeater. We propose a different model to explain the changing supernova remnant morphology and the positions of the luminous blue variable and the bursting source.
Where is SGR1806-20? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.If you have personal experience with Where is SGR1806-20?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Where is SGR1806-20? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-560852