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Back Artist's impression of a highly obscured high-mass X-ray binary

Artist's impression of a highly obscured high-mass X-ray binary


Date: 03 March 2013
Satellite: INTEGRAL
Depicts: Artist's impression of a neutron star in a highly obscured high-mass X-ray binary
Copyright: ESA/AOES Medialab

This image shows an artist's impression of a highly obscured high-mass X-ray binary, consisting of a neutron star that is accreting mass from its companion, a blue supergiant star.

Highly obscured high-mass X-ray binaries exhibit very faint emission at soft X-ray energies and as a result had eluded searches in this portion of the electromagnetic spectrum. They were discovered in 2003 via hard X-ray observations with INTEGRAL. Astronomers believe that the soft X-rays are absorbed by the wind released by the companion star, which embeds the neutron star.

Last Update: 1 September 2019
17-Mar-2026 02:51 UT

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