Science with the World Space Observatory - Ultraviolet

Ana I. Gomez de Castro; Isabella Pagano; Mikhail Sachkov; Alain Lecavelier; Giampaolo Piotto; Rosa Gonzalez; Boris Shustov

doi:10.1007/978-0-387-87621-4_42

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arXiv · 0811.0316

Science with the World Space Observatory - Ultraviolet

Ana I. Gomez de Castro·Isabella Pagano·Mikhail Sachkov·Alain Lecavelier·Giampaolo Piotto·Rosa Gonzalez·Boris Shustov

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Abstract

The World Space Observatory-Ultraviolet (WSO-UV) will provide access to the UV range during the next decade. The instrumentation on board will allow to carry out high resolution imaging, high sensitivity imaging, high resolution (R~55000) spectroscopy and low resolution (R~2500) long slit spectroscopy. In this contribution, we briefly outline some of the key science issues that WSO-UV will address during its lifetime. Among them, of special interest are: the study of galaxy formation and the intergalactic medium; the astronomical engines; the Milky Way formation and evol ution, and the formation of the Solar System and the atmospheres of extrasolar p lanets.

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Ana I. Gomez de Castro, Isabella Pagano, Mikhail Sachkov, Alain Lecavelier, Giampaolo Piotto, Rosa Gonzalez, Boris Shustov. 2008-11-03. Science with the World Space Observatory - Ultraviolet. https://doi.org/10.1007/978-0-387-87621-4_42

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