TY  - JOUR
AU  - Gómez De Castro, Ana Inés
AU  - Lamzin, Sergei A.
PY  - 2011
DO  - 10.1007/s10509-011-0649-2
SN  - 0004-640X
UR  - https://hdl.handle.net/20.500.14352/42230
T2  - Astrophysics and space science
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...
LA  - eng
M2  - 61
PB  - Springer
KW  - T-tauri stars
KW  - Herbig ae/be stars
KW  - Young stars
KW  - Ab-aurigae
KW  - Mg-ii
KW  - Dense outflows
KW  - Bp tauri
KW  - Ultraviolet
KW  - Accretion
KW  - Line
TI  - Pre main sequence stars as UV sources for the World Space Observatory-UV mission
TY  - journal article
VL  - 335
ER  -