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Astrophysical Journal, ISSN 0004-637X, 08/2016, Volume 827, Issue 1, pp. 41 - 41
The region around SGR 1806-20 and its host stellar cluster Cl* 1806-20 is a potentially important site of particle acceleration. The soft [gamma]-ray repeater... 
stars: magnetars | cosmic rays | pulsars: individual (SGR 1806-20) | ISM: individual objects (SNR G9.7-0.0, HESS J1808-204, W31) | Supernova remnants | Telescopes | Flux | Emission | Centroids | Spectra | Variable stars | Massive stars
Journal Article
Nature, ISSN 0028-0836, 04/2005, Volume 434, Issue 7037, pp. 1107 - 1109
Two classes of rotating neutron stars-soft γ-ray repeaters (SGRs) and anomalous X-ray pulsars-are magnetars, whose X-ray emission is powered by a very strong... 
OUTBURSTS | RADIATIVE MECHANISM | MISSION | MULTIDISCIPLINARY SCIENCES | REPEATER SGR 1900+14 | BURST | 1998 AUGUST 27 | Gamma rays | Solar flares | Gamma ray astronomy
Journal Article
Nature, ISSN 0028-0836, 04/2005, Volume 434, Issue 7037, pp. 1098 - 1103
Soft-gamma-ray repeaters (SGRs) are galactic X-ray stars that emit numerous short-duration (about 0.1 s) bursts of hard X-rays during sporadic active periods.... 
1979 MARCH 5 | SGR 1900+14 | RADIATIVE MECHANISM | REPEATERS | MULTIDISCIPLINARY SCIENCES | X-RAY | MAGNETIZED NEUTRON-STARS | LBV 1806-20 | SPECTRUM | 1998 AUGUST 27 | GIANT FLARE | Gamma rays | Solar flares | Gamma ray astronomy
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 10/2011, Volume 740, Issue 2, p. 55
In 2004, SGR 1806-20 underwent a period of intense and long-lasting burst activity that included the giant flare of 2004 December 27-the most intense... 
X-rays: bursts | pulsars: individual (SGR 1806?20) | X-RAY OSCILLATIONS | ASTRONOMY & ASTROPHYSICS | STATISTICAL PROPERTIES | GIANT FLARE | SGR-1806-20 | EMISSION | pulsars: individual (SGR 1806-20) | GAMMA-REPEATER SGR-1900+14 | DISCOVERY | Physics - High Energy Astrophysical Phenomena
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2015, Volume 809, Issue 2, pp. 1 - 8
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2016, Volume 827, Issue 1, pp. 59 - 59
Journal Article
Astrophysical Journal, ISSN 0004-637X, 12/2017, Volume 851, Issue 1
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2011, Volume 415, Issue 3, pp. 2485 - 2494
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2005, Volume 433, Issue 2, pp. L13 - L16
We present the results of an analysis of the quiescent X-ray emission from the Soft Gamma-Ray Repeater SGR 1806- 20, taken during an INTEGRAL ultra-deep survey... 
Stars: individual: SGR 1806-20 | Gamma rays: bursts | Pulsars: general | pulsars : general | CYCLOTRON-RESONANCE | COUNTERPART | SOFT GAMMA REPEATER | X-RAY PULSAR | TIME HISTORIES | gamma rays : bursts | DISCOVERY | SGR 1806-20 | stars : individual : SGR 1806-20 | CATALOG | ASTRONOMY & ASTROPHYSICS | HIGH-ENERGY TRANSIENT | MAGNETIC-FIELD
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 2010, Volume 509, Issue 1, p. A99
Context. The 2004 december 27 giant flare from SGR 1806-20 produced a radio nebula that was detectable for weeks. It was observed at a wide range of radio... 
Neutron - Radio continuum | SGR 1806-20 - Stars | Individual | Stars | stars: individual: SGR 1806-20 | radio continuum: stars | COUNTERPART | ASTRONOMY & ASTROPHYSICS | AFTERGLOW | STARS | VLA | MASS-LOSS | SPECTRUM | GAMMA-RAY BURSTS | MAGNETAR SGR-1806-20 | stars: neutron
Journal Article
Journal of High Energy Astrophysics, ISSN 2214-4048, 09/2014, Volume 3-4, pp. 41 - 46
Diffuse radio emission was detected around the soft gamma-ray repeater SGR 1806-20  after its 2004 powerful giant flare. We study the possible extended X-ray... 
magnetars | Pulsar | magnetic fields | individual, SGR 1806-20 | Stars | X-rays | Pulsar, individual, SGR1806-20 | X-rays, stars | Stars, magnetic fields | Stars, magnetars
Journal Article
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