- Supergiant Fast X-ray Transients -
 

ESA PRESS RELEASE
TRADUCCIÓN AL ESPAÑOL

We have recently discovered a new kind of high mass X-ray binaries which may represent a major subclass. These objects are characterised by the occurrence of very fast X-ray outbursts. Most of the time, they are not detected as X-ray sources or only detected as a waek source. Occasionally, they flare up and, for a very brief period of time, emit strong hard X-ray radiation. Because of the brevity of the outbursts, these X-ray sources had been dubbed fast X-ray transients. Our recent work has shown that, at least a significant fraction of them, are associated with supergiant stars, huge stars that represent the final phase in the life of stars much more massive than the Sun. The connection between supergiant stars and fast transients was rather unexpected. We have called these objects Supergiant Fast X-ray Transients.


artist's impression


Relevant Papers




Transient X-ray sources

For an introduction to celestial X-ray sources, check out the X-ray binary page.

Some X-ray sources are not normally detected, or are normally observed as very weak sources, but occasionally display 'outbursts', that is, short periods of activity during which X-ray emission is much stronger. Scientists call these sources transient. Thanks to the capabilities of ESA's gamma-ray observatory INTEGRAL, combined with other space-born X-ray observatories and ground telescopes, a new kind of transients, known as "Supergiant Fast  X-ray Transients" has been discovered.


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Written and maintained by Ignacio N.. Last update on 13th February2008.