Abstract
A good diagnostic for the presence of hot thin plasmas is their emission in the far UV and x-ray bands. For this reason, high quality x-ray observations of normal galaxies should provide us with the right tool to detect directly hot extragalactic gas in these systems.
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© 1988 Kluwer Academic Publishers
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Trinchieri, G. (1988). Observations of Galaxies and Galactic Halos. In: Pallavicini, R. (eds) Hot Thin Plasmas in Astrophysics. NATO ASI Series, vol 249. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3065-0_17
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DOI: https://doi.org/10.1007/978-94-009-3065-0_17
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