Possible NIR counterpart to the AXP 1E 1547.0-5408

Authors
  • R.P. Mignani
  • N. Rea
  • G.L. Israel
  • V. Testa
Publication date 2008
Journal The astronomer's telegram
Volume | Issue number 1758
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
On 2008 October 3rd, Swift-BAT triggered on several short bursts from the direction of the Anomalous X-ray Pulsar (AXP) 1E1547.0-5408 (Krimm et al. GCN 8311, 8312; Rea et al. Atel #1756). This is the second known transient radio AXP discovered to date (Gelfand & Gaensler 2007; Camilo et al. 2007), and it showed the previous X-ray outburst around June 2007 (Halpern et al. 2008). During the decay of the 2007 X-ray outburst we observed 1E 1547.0-5408 in the Ks band (on 2007 July 8th, 12th, and August 17th) with the NAOS -CONICA (NACO) instrument mounted at the ESO- VLT (Mignani, Rea, Testa, et al., 2008 submitted).
Document type Article
Language English
Published at http://www.astronomerstelegram.org/?read=1758
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