IGR J18483-0311: an accreting X-ray pulsar observed by INTEGRAL

2007/02/19 by V. Sguera, A. B. Hill, A. J. Bird +9 · 5 citations
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astrophysical Phenomena and Observations #Pulsars and Gravitational Waves Research #astro-ph

paper · pdf · doi:10.1051/0004-6361:20066762

accepted for publication in A&A, 10 pages, 17 figures, 4 tables

arxiv created 2007/02/19 · openalex publication_date 2007/02/20 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31

Abstract

Context.IGR J18483-0311 is a poorly known transient hard X-ray source discovered by INTEGRAL during observations of the Galactic Center region performed between 23–28 April 2003.

Citations

• Studies in astronomical time series analysis. II - Statistical aspects of spectral analysis of unevenly spaced data
• The Two Micron All Sky Survey (2MASS)

Cited by

• Discovery of the 51.47-d orbital period in the supergiant fast X-ray transient XTE J1739−302 with INTEGRAL
• Multi-wavelength observations of Galactic hard X-ray sources discovered byINTEGRAL
• The supergiant fast X-ray transients XTE J1739-302 and IGR J08408-4503 in quiescence withXMM-Newton
• Swift observations of IGR J16479-4514 in outburst
• IGR J18483–0311: a new intermediate supergiant fast X-ray transient
• Population of persistent high-mass X-ray binaries in the Milky Way