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In search of a new era of UK X-ray astronomy

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journal contribution
posted on 2018-05-15, 13:40 authored by Poshak Gandhi, Nathalie Degenaar, Chris Done, Mike G. Watson
X-ray astronomy is our gateway to the hot universe. More than half of the baryons in the cosmos are too hot to be visible at shorter wavelengths. Studying the extreme environments of black hole and neutron star vicinities also requires X-ray data. With the successful launch of India's AstroSat in 2015, and the few – but transformative – results from Japan's short-lived Hitomi mission in 2016, a new window has been opened into high-sensitivity fast timing and high X-ray spectral resolution. Together with the all-sky survey missions expected soon, X-ray astronomy is now exploring new parameter space.

History

Citation

Astronomy and Geophysics, 2017, 58 (6), pp. 6.24-6.28

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • VoR (Version of Record)

Published in

Astronomy and Geophysics

Publisher

Oxford University Press

issn

1366-8781

eissn

1468-4004

Copyright date

2017

Available date

2018-05-15

Publisher version

https://academic.oup.com/astrogeo/article/58/6/6.24/4638408

Language

en

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