Searching for small-scale diffuse emission around SGR 1806-20
Author:
Funder
NewCompstar
NWO
Publisher
Elsevier BV
Subject
Astronomy and Astrophysics,Space and Planetary Science
Reference28 articles.
1. Detection of a radio counterpart to the 27 December 2004 giant flare from SGR 1806-20;Cameron;Nature,2005
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3. Formation of very strongly magnetized neutron stars – implications for gamma-ray bursts;Duncan;Astrophys. J. Lett.,1992
4. SGR 1806-20 about two years after the giant flare: Suzaku, XMM-Newton and INTEGRAL observations;Esposito;Astron. Astrophys.,2007
5. Structure in the radio counterpart to the 2004 December 27 giant flare from SGR 1806-20;Fender;Mon. Not. R. Astron. Soc.,2006
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1. Extended VHE γ-ray emission towards SGR1806−20, LBV 1806−20, and stellar cluster Cl* 1806−20;Astronomy & Astrophysics;2018-04
2. Pulsar-Wind Nebulae and Magnetar Outflows: Observations at Radio, X-Ray, and Gamma-Ray Wavelengths;Space Science Reviews;2017-03-30
3. Pulsar-Wind Nebulae and Magnetar Outflows: Observations at Radio, X-Ray, and Gamma-Ray Wavelengths;Jets and Winds in Pulsar Wind Nebulae, Gamma-Ray Bursts and Blazars;2017
4. On the possible wind nebula of magnetar Swift J1834.9–0846: a magnetism-powered synchrotron nebula;Research in Astronomy and Astrophysics;2016-08-30
5. THE WIND NEBULA AROUND MAGNETAR SWIFT J1834.9–0846;The Astrophysical Journal;2016-06-22
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