No radio pulsations detected from SGR 1627-41 following renewed X- ray activity

Details No radio pulsations detected from SGR 1627-41 following renewed X- ray activity No radio pulsations detected from SGR 1627-41 following renewed X- ray activity

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1558....1c&link_type=abstract

The Astronomer's Telegram, #1558

Astronomy and Astrophysics

Astronomy

4

Radio, X-Ray, Neutron Stars, Pulsars, Soft Gamma-Ray Repeaters, Transients

Scientific paper

Starting on May 28, 2008, the SGR 1627-41 displayed X-ray bursting and enhanced flux after nearly 10 years of relative inactivity (ATEL #1548, #1549, #1555). Two magnetars are known to emit radio pulses (Camilo et al. 2007, ApJ, 666, L93), and in at least one case these are transient and have followed an X-ray outburst after many years in quiescence (Camilo et al. 2006, Nature, 442, 892). Therefore, although previous radio searches of SGR 1627-41 have been unsuccessful, we are searching for radio emission following its recent renewed burst of activity.

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