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- W2020549522 endingPage "147" @default.
- W2020549522 startingPage "137" @default.
- W2020549522 abstract "In 2006 February, shortly after its launch, Swift began monitoring the center of the Milky Way with the on board X-Ray Telescope using short 1-ks exposures performed every 1–4 days. Between 2006 and 2014 over 1200 observations have been obtained, accumulating to ≃1.3Ms of exposure time. This has yielded a wealth of information about the long-term X-ray behavior of the supermassive black hole Sgr A⁎, and numerous transient X-ray binaries that are located within the 25′×25′ region covered by the campaign. In this review we highlight the discoveries made during these first nine years, which include 1) the detection of seven bright X-ray flares from Sgr A⁎, 2) the discovery of the magnetar SGR J1745–29, 3) the first systematic analysis of the outburst light curves and energetics of the peculiar class of very-faint X-ray binaries, 4) the discovery of three new transient X-ray sources, 5) the exposure of low-level accretion in otherwise bright X-ray binaries, and 6) the identification of a candidate X-ray binary/millisecond radio pulsar transitional object. We also reflect on future science to be done by continuing this Swift's legacy campaign, such as high-cadence monitoring to study how the interaction between the gaseous object ‘G2’ and Sgr A⁎ plays out in the future." @default.
- W2020549522 created "2016-06-24" @default.
- W2020549522 creator A5013480528 @default.
- W2020549522 creator A5020825353 @default.
- W2020549522 creator A5031344818 @default.
- W2020549522 creator A5076019304 @default.
- W2020549522 creator A5080365085 @default.
- W2020549522 creator A5087214327 @default.
- W2020549522 date "2015-09-01" @default.
- W2020549522 modified "2023-10-18" @default.
- W2020549522 title "The Swift X-ray monitoring campaign of the center of the Milky Way" @default.
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