The Growth, Polarization, and Motion of the Radio Afterglow From the Giant Flare From SGR 1806-20

Astrophysical Journal - United States
doi 10.1086/491648
Full Text
Abstract

Available in full text

Date
Authors
Publisher

IOP Publishing

Related search

The Calm After the Storm: XMM-Newton Observation of SGR 1806–20 Two Months After the Giant Flare of 2004 December 27

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2005English

The Connection Between W31, SGR 1806–20, and LBV 1806–20: Distance, Extinction, and Structure

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Proper Motions and Origins of SGR 1806–20 and SGR 1900+14

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Quasi-Periodic Oscillations in Short Recurring Bursts of Magnetars SGR 1806–20 and SGR 1900+14 Observed Withrxte

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

Polarization of Photoneutrons From the Giant Resonance.

1967English

On the Possibility of Observing Radio Emission From Flare Stars

Symposium - International Astronomical Union
1959English

Combining Visibilities From the Giant Meterwave Radio Telescope and the Nancay Radio Heliograph

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2006English

The Polarization Evolution of the Optical Afterglow of GRB 030329

AIP Conference Proceedings
AstronomyPhysics
2004English

Radio Linear and Circular Polarization From M81*

Journal of Physics: Conference Series
AstronomyPhysics
2006English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy