2006/11/07 by S. Campana, N. Rea, G. L. Israel +2 · 5 citations
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysical Phenomena and Observations #Binary pulsar #Earth Systems and Cosmic Evolution #Flux (metallurgy) #Luminosity #Magnetic flux #Magnetosphere #Pulsar #Pulsars and Gravitational Waves Research #Spectral line #Spectral properties #astro-ph
paper · pdf · doi:10.1051/0004-6361:20065482
6 pages, 5 figures, accepted for publication on A&A
arxiv created 2006/11/07 · openalex publication_date 2006/12/18 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Convincing evidence of long-term variations in the emission properties of the anomalous X-ray pulsar 1RXS J170849.0–400910 has been gathered in the past few years. In particular, and following the pulsar glitches of 1999 and 2001, XMM-Newton witnessed a decline in 2003 of the X-ray flux accompanied by a definite spectral softening. This suggested the existence of a correlation between the luminosity and the spectral hardness in this source, similar to what was seen in the soft γ-repeater SGR 1806–20. Here we report on new Chandra and Swift observations of 1RXS J170849.0–400910 performed in 2004 and 2005, respectively. These observations confirm and strengthen the proposed correlation. The trend appears to have now reversed: the flux has increased and the spectrum is now harder. We briefly discuss the consequences of these observations for the twisted magnetosphere scenario for anomalous X-ray pulsars.