The Proper Motion of SGR1900+14

Details The Proper Motion of SGR1900+14 The Proper Motion of SGR1900+14

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.9506h&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #95.06; Bulletin of the American Astronomical Society, Vol. 33, p.1446

Astronomy and Astrophysics

Astronomy

Scientific paper

The magnetar model predicts that soft gamma repeaters may be born with high velocities, and SGR1900+14 appears to be an extreme example of this. Its transverse motion in fact appears to be so large that it can be measured by comparing a single Chandra observation to previous radio observations of this source. We have now conducted a 30 ksec observation of the source with Chandra. Data analysis is currently underway, and we will report on the latest results here.

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