Anomalous X-Ray Pulsar: Difference between revisions
From Star Trek : Freedom's Wiki
Nicesociety (talk | contribs) (Created page with 'thumb|250px|right|An Anomalous X-ray Pulsar.jpg Anomalous X-ray Pulsars (AXPs) are now widely believed to be Magnetars —young, isol…') |
Nicesociety (talk | contribs) No edit summary |
||
| Line 1: | Line 1: | ||
[[File:Anomalous X-ray Pulsar.jpg|thumb|250px|right|An Anomalous X-ray Pulsar.jpg]] | [[File:Anomalous X-ray Pulsar.jpg|thumb|250px|right|An Anomalous X-ray Pulsar.jpg]] | ||
[[Anomalous X-ray Pulsar]]s (AXPs) are now widely believed to be [[Magnetar]]s —young, isolated, highly magnetized [[Neutron Star]]s. These energtic X-ray pulsars are characterized by slow rotation periods of ~2–12 seconds and large magnetic fields of ~1013–1015 | [[Anomalous X-ray Pulsar]]s (AXPs) are now widely believed to be [[Magnetar]]s —young, isolated, highly magnetized [[Neutron Star]]s. These energtic X-ray pulsars are characterized by slow rotation periods of ~2–12 seconds and large magnetic fields of ~1013–1015 [[Gauss]] (1 to 100 [[Tesla|Gigatesla]]s). There are currently 9 known and 1 candidate AXPs. The identification of AXPs with magnetars was motivated by their similarity to another enigmatic class of sources, the [[Soft Gamma Repeater]]s. | ||
[[Category: Stars and Stellar Phenomenon]][[Category: Science]] | [[Category: Stars and Stellar Phenomenon]][[Category: Science]] | ||
Revision as of 16:42, 4 March 2010
Anomalous X-ray Pulsars (AXPs) are now widely believed to be Magnetars —young, isolated, highly magnetized Neutron Stars. These energtic X-ray pulsars are characterized by slow rotation periods of ~2–12 seconds and large magnetic fields of ~1013–1015 Gauss (1 to 100 Gigateslas). There are currently 9 known and 1 candidate AXPs. The identification of AXPs with magnetars was motivated by their similarity to another enigmatic class of sources, the Soft Gamma Repeaters.
