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


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Resumen

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.


Tipo de documento:Artículo
Palabras clave:T-tauri stars; herbig ae/be stars; young stars; ab-aurigae; mg-ii; dense outflows; bp tauri; ultraviolet; accretion; line
Materias:Ciencias > Matemáticas > Astronomía
Código ID:15860
Depositado:06 Jul 2012 11:07
Última Modificación:06 Feb 2014 10:33

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