Magnetar Observations in the Swift-Fermi Era Contributor(s): Nasa Technical Reports Server (Ntrs) (Created by), Kouveliotou, Chryssa (Author) |
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ISBN: 1289039127 ISBN-13: 9781289039127 Publisher: Bibliogov OUR PRICE: $14.96 Product Type: Paperback - Other Formats Published: June 2013 |
Additional Information |
BISAC Categories: - Political Science |
Physical Information: 0.09" H x 7.44" W x 9.69" (0.21 lbs) 44 pages |
Descriptions, Reviews, Etc. |
Publisher Description: This slide presentation reports on the current status of Magnetar observations, and on the results combining multi-satellite. Magnetars are magnetically powered neutron stars. There is discussion about several Soft Gamma Repeaters (SGR) also known as Magnetars, though there aer other neutron stars that may be considered as magnetars (i.e., Anomalous X-ray Pulsars (AXPs) Dim Isolated Neutron Stars (DINs) Compact Central X-ray Objects (CCOs) Rotation Powered Pulsars.) An example of a Rotation Powered PSRs, (i.e., PSR J1846-0258) is reviewed, and examples of SGRs are reviewed (i.e., SGR 0501+4516, SGR 0501+4516, SGR J1550-5418, and SGR 0418+5729). There is also discussion about Photospheric Radius Expansion (PRE) in thermonuclear bursts. |