2006/08/24 by S. Fritz, I. Kreykenbohm, J. Wilms +5 · 2 citations
Earth and Planetary Sciences · Physics and Astronomy · #Accretion (finance) #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #Binary star #Computational astrophysics #Earth Systems and Cosmic Evolution #Focus (optics) #Neutron star #Pulsar #Torque #X-ray pulsar #astro-ph
paper · pdf · doi:10.1051/0004-6361:20065557
Accepted for publication in Astronomy & Astrophysics, 11 pages, 8 figures
arxiv created 2006/08/24 · openalex publication_date 2006/08/25 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims.We present an analysis of the accreting X-ray pulsar system 4U 1907+09 based on INTEGRAL data. The main focus of this analysis is a study of the timing behavior of this source. In addition we also show an analysis of the 5–90 keV spectrum.