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Pre main sequence stars as UV sources for the World Space Observatory-UV mission

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Gómez de Castro, Ana Inés and Lamzin, Sergei A. (2011) Pre main sequence stars as UV sources for the World Space Observatory-UV mission. Astrophysics and space science, 335 (1). pp. 61-68. ISSN 0004-640X

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Official URL: http://www.springerlink.com/content/mk71847u6n384761/fulltext.pdf


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Abstract

Pre-main sequence stars are bright UV (UV) sources compared with their main sequence analogues. The source of this excess is the high energy processes associated with the physics of accretion/outflow during early stellar evolution. In this review, the main sources of UV excess are described as well as the most significant "unknowns" in the field. Special emphasis is made on the results from the last observations carried out with the Hubble Space Telescope and on the relevance of future dedicated monitoring programs with the World Space Observatory-UV.


Item Type:Article
Uncontrolled Keywords:T-tauri stars; herbig ae/be stars; young stars; ab-aurigae; mg-ii; dense outflows; bp tauri; ultraviolet; accretion; line
Subjects:Sciences > Mathematics > Astronomy
ID Code:15860
Deposited On:06 Jul 2012 11:07
Last Modified:26 Jun 2018 07:28

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