Abstract
Recently, with the Chandra X-ray Telescope we have detected several local X-ray absorption lines along lines-of-sight towards distant quasars. These absorption lines are produced by warm/hot gas located in local intergalactic space and/or in our Galaxy. I will present our observations and discuss the origin of the X-ray absorption and its implications in probing the warm/hot component of local baryons.
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Fang, T., Canizares, C., Sembach, K., Marshall, H., Lee, J., Davis, D. (2004). Chandra Detection of X-ray Absorption from Local Warm/Hot Gas. In: Lieu, R., Mittaz, J. (eds) Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena. Astrophysics and Space Science Library, vol 309. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-2564-8_8
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DOI: https://doi.org/10.1007/978-1-4020-2564-8_8
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