Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-08-10
Astronomy and Astrophysics
Astrophysics
16 pages, 4 figures, accepted by ApJ
Scientific paper
10.1086/324339
We present observations of the Soft Gamma-ray Repeater SGR 1806-20 taken with the Chandra X-ray Observatory. We identify the X-ray counterpart of SGR 1806-20 based on detection of 7.5-s pulsations. Using three unrelated X-ray sources (and USNO stars) as position references, we are able to determine that the SGR is at alpha_{2000}=18h08m39.32s and delta_{2000}=-20o24'39.5", with rms uncertainty of 0.3" in each coordinate. We find that SGR 1806-20 is located within the 1-sigma error region determined by Interplanetary Network data and is 14+/-0.5 arcsec distant from the non-thermal core of SNR G10.0-0.3, excluding SGR 1806-20 as the origin of the core. We see evidence for a significant deviation of the spin-down of SGR 1806-20 from its long-term trend, demonstrating erratic spin-down behavior in this source similar to that seen in other SGRs. Finally, we show that there is a broad X-ray halo surrounding SGR 1806-20 out to radii ~1' due to scattering in the interstellar medium.
Fox Derek W.
Frail Dale A.
Gotthelf Eric Van
Kaplan David L.
Kulkarni Sanjeev R.
No associations
LandOfFree
Precise Chandra Localization of the Soft Gamma-ray Repeater SGR 1806-20 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 Precise Chandra Localization of the Soft Gamma-ray Repeater SGR 1806-20, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Precise Chandra Localization of the Soft Gamma-ray Repeater SGR 1806-20 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-177659