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- W112367069 abstract "The X-ray sky is extremely variable. Transient sources occur on probably all timescales. Historically, the easiest timescales to study are seconds to minutes, and days to months. Most of these transients are Galactic in origin and have been shown to be powered by gravitational energy release during accretion of matter onto a compact object or by thermonuclear runaway processes on neutron stars (see Chapter 3 by Strohmayer and Bildsten). Less well understood are the transients with timescales between a minute and a day, the so-called “fast X-ray transients” (FXTs). These often occur off the Galactic plane and are, therefore, sometimes also referred to as “high latitude transients” (see Fig. 6.1). In general an FXT is loosely defined as a new temporary X-ray source that disappears on a timescale of less than a day and is not related to a known persistent X-ray source. The term, however, has been used as a repository for all sorts of ill-understood flares, bursts, flashes and related phenomena." @default.
- W112367069 created "2016-06-24" @default.
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- W112367069 date "2006-04-06" @default.
- W112367069 modified "2023-09-25" @default.
- W112367069 title "Fast X-ray transients and X-ray flashes" @default.
- W112367069 doi "https://doi.org/10.1017/cbo9780511536281.007" @default.
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