TY  - JOUR
AU  - Gómez De Castro, Ana Inés
AU  - López Santiago, Javier
AU  - Talavera, A.
AU  - Sytov, A. Y.
AU  - Bisikalo, D.
PY  - 2013
DO  - 10.1088/0004-637X/766/1/62
SN  - 0004-637X
UR  - https://hdl.handle.net/20.500.14352/33291
T2  - Astrophysical journal
AB  - AK Sco stands out among pre-main-sequence binaries because of its prominent ultraviolet excess, the high eccentricity of its orbit, and the strong tides driven by it. AK Sco consists of two F5-type stars that get as close as 11 R-* at periastron...
LA  - eng
PB  - IOP Publishing
KW  - Binaries: spectroscopic
KW  - Magnetic fields
KW  - Stars: pre-main sequence
KW  - T-tauri stars
KW  - X-ray-emission
KW  - System kh 15d
KW  - Wavelength dependence
KW  - Accretion shocks
KW  - mg-ii
KW  - Scorpii
KW  - Polarization
KW  - Simulations
KW  - Extinction
TI  - XMM-Newton monitoring of the close pre-main-sequence binary AK Sco. Evidence of tide-driven filling of the inner gap in the circumbinary disk
TY  - journal article
VL  - 766
ER  -