RT Journal Article
T1 Pre main sequence stars as UV sources for the World Space Observatory-UV mission
A1 Gómez De Castro, Ana Inés
A1 Lamzin, Sergei A.
AB 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.
PB Springer
SN 0004-640X
YR 2011
FD 2011-09
LK https://hdl.handle.net/20.500.14352/42230
UL https://hdl.handle.net/20.500.14352/42230
LA eng
NO Gómez de Castro, A. I. & Lamzin, S. A. «Pre Main Sequence Stars as UV Sources for the World Space Observatory-UV Mission». Astrophysics and Space Science, vol. 335, n.o 1, septiembre de 2011, pp. 61-68. DOI.org (Crossref), https://doi.org/10.1007/s10509-011-0649-2.
NO Ministerio de Ciencia, Innovación y Universidades (España)
DS Docta Complutense
RD 9 abr 2025