TW And     HIP d=232(67) pc, periodic variable; magnetic activity and evolution 
TW And      (And_12); status of evolution (And_7); radio emission (And_13).
UU And     Period jumps (And_2).
WW And     Accretion disk (And_14); radio emission (And_15, And_16).
XZ And     Period change (And_17, And_18, And_4); radio emission (And_15). 
AA And     Periodic variable (HIP).
DW Aps     HIP d=490(280) pc, periodic variable; radio emission (Aps_1).
RY Aqr     Different absolute parameters (B&D); magnetic activity and evolution
RY Aqr      (Aqr_3, Aqr_4); radio emission (Aqr_5).
CZ Aqr     Period change (Aqr_6).
XZ Aql     Period change (Aql_1).
YZ Aql     Extrasolar planet (Aql_10).
FK Aql     Period change (Aql_11).
KO Aql     HIP d=265(75) pc, periodic variable; radio emission (Aql_12, Aql_13);
KO Aql      mass transfer (Aql_14).
QY Aql     Extrasolar planet (Aql_10); radio emission (Aql_13).
V342 Aql   Duplicity-induced variability (HIP); mass flow (Aql_15); accretion
V342 Aql    disks (Aql_16).
V346 Aql   Mass transfer (Aql_14); radio emission (Aql_12).
R Ara      HIP d=80+/-13pc and multiple system; d=166.7 pc and X-ray emission
R Ara       (Ara_5); radio emission (Ara_6).
RW Ara     Radio emission (Ara_6); mass transfer (Ara_7).
SX Aur     HIP d=320(140) pc and periodic variable; d=1200(200) pc (Aur_3);
SX Aur      different absolute parameters (Aur_1); reversals of mass transfer
SX Aur      (Aur_8).
AK Aur     Visual companion (Aur_9).
AM Aur     Radio continuum emission (Aur_10; Aur_11; Aur_12).
IM Aur     d=359 pc (Aur_4); d=434.8 pc (Aur_7); complex period variations
IM Aur      (Aur_13); H? mass transfer structures (Aur_14); apsidal motion
IM Aur      (Aur_15; Aur_16); radio emission (Aur_17); X-ray emission (Aur_7).
Y Cam      HIP periodic variable; pulsating component in the system (Cam_4);
Y Cam       possibly 4-body system (Cam_5).
SS Cam     HIP d=320(180) pc, periodic variable, new classified; X-ray 
SS Cam      variability (Cam_7).
S Cnc      HIP d=340(130) pc and periodic variable; radio emission (Cnc_3); 
S Cnc       X-ray emission (Cnc_4).
RY Cnc     Probably periodic variable (KKN).
RZ Cnc     HIP d=310(150)pc and periodic variable; circumstellar matter (Cnc_7);
RZ Cnc      chromospherically active binary (Cnc_8).
RU Cnc     HIP d=330(170) pc and periodic variable; differential rotation and
RU Cnc      activity cycle (Cnc_9); only photoelectric observations 
RU Cnc      (Cnc_10, Cnc_11).
TU Cnc     Possible mass and angular momentum loss (Cnc_12).
R CMa      Third body (CMa_10).
AK CMi     Period change (CMi_1).
RX Cas     HIP  d=330(190) pc; W-Ser type (Cas_22); 
RX Cas      Very fast mass transfer (Cs_3).
RZ Cas     HIP d=62.5(2.4) pc; Frequent unpredictable period variations (Cas_4);
RZ Cas      A possible thirdbody (Cas_5). Third body or apsidal motion (Cas_17).
RZ Cas      Low level of magnetic activity (Cas_17).
SX Cas     Third body (Cas_19); System, enduring slow mass transfer (Cas_24).
TV Cas     HIP d=254(49) pc; Period variation (Cas_20).
AB Cas     HIP d=300(120) pc; Eclipsing binary with pulsating components 
AB Cas      (Cas_25, Cas_26), Mass transfer and third body from O-C analysis 
AB Cas      (Cep_27).
DO Cas     HIP d=147(21) pc.
CT Cen     TYC d=56(49) pc.
V379 Cen   HIP d=231(72) pc.
U Cep      HIP d=207(23) pc; Disk structure (Cep_20); Variable mass transfer
U Cep       activity (Cep_21), Complex orbital period variation (Cep_1, KKN).
RS Cep     Circumstellar matter (Cep_16); Orbital period variation (Cep_22, KKN)
XX Cep     HIP d=314(93) pc; Third body (Cep_23), Orbital period variation (KKN)
XY Cep     HIP d=340(140) pc, Orbital period variation (KKN).
EK Cep     HIP d=153(14) pc; Apsidal motion and the secondary component seems to
EK Cep      be in the pre-main sequence phase (Cep_24, KKN).
AT Cir     HIP d=168(25) pc and periodic variable.
RW CrA     HIP periodic variable.
V681 CrA   HIP d= 219(45) pc.
U CrB      HIP d=338(95) pc, periodic variable; third body (CrB_1); UPS
U CrB       photoelectric observations (CrB_2).
RW CrB     HIP d= 196(63) pc, periodic variable; possible mass and angular
RW CrB      momentum loss (CrB_6).
SW Cyg     Period jumps (Cyg_33); period changes (Cyg_34, Cyg_35, Cyg_36);
SW Cyg      accretion disk (Cyg_37).
SY Cyg     Apsidal motion (Cyg_29).
UW Cyg     TYCHO d=20 pc.
VW Cyg     HIP d=610 pc.
WW Cyg     HIP d=740 pc;  period change (Cyg_38); accretion disk (Cyg_39).
ZZ Cyg     Delta Scuti type physical  variability of the hotter component 
ZZ Cyg      (Cyg_40).
CG Cyg     RSCVn, period change (Cyg_41, Cyg_42, Cyg_43). 
KU Cyg     Accretion disk (Cyg_44, Cyg_16, Cyg_45, Cyg_46). 
MY Cyg     Displeced secondary minimum (Cyg_25).
V463 Cyg   Displeced secondary minimum (Cyg_25) third light (Cyg_17).
V512 Cyg   Displeced secondary minimum (Cyg_25).
V753 Cyg   Accretion disk (Cyg_39).
V909 Cyg   Triple star (Cyg_47).
V959 Cyg   Displeced secondary minimum (Cyg_25).
V1898 Cyg  HIP d=620 pc.
V2080 Cyg  HIP d=79.4 pc.
W Del      Accretion disk (Del_10); apsidal motion (Del_9).
TT Del     Period change (Del_11). 
FZ Del     Period change (Del_12); eccentric orbit (Del_13).
Z Dra      HIP d=236 pc.
RR Dra     Period change, period jumps (Dra_20); accretion disk (Dra_21).
RZ Dra     HIP d=550 pc; third body, period change (Dra_8).
TW Dra     HIP d=122 pc; third body, period change (Dra_22); accretion disk
TW Dra     (Dra_21).
AI Dra     HIP d=142 pc; period change, third body (Dra_10) accretion disk
AI Dra      (Dra_21).
BF Dra     HIP d=560 pc; system with eccentric orbit (Dra_6).
S Equ      HIP d=400 pc; third body from light curva analysis (Equ_1); mass
S Equ       transfer and third body from O-C analysis (Equ_7, Equ_8).
AS Eri     HIP d=228 pc.
RW Gem     HIP d=95 pc.
RX Gem     Period change (Gem_14); third body (Gem_15); accretion disk (Gem_16,
RX Gem      Gem_17).
RY Gem     Accretion disk (Gem_18, Gem_17).
AF Gem     Triple star (Gem_19).
AY Gem     Period change (Gem_20).
BD Gem     Accretion disk (Gem_17).
X Gru      Period change  (Gru_1).
U Her      HIP d=265(39) pc.
SZ Her     HIP d=216(57) pc.
UX Her     HIP d=209(50) pc.
V338 Her   HIP d=380(150) pc.
SX Hya     HIP d= 245(71) pc.
TT Hya     HIP d= 154(22) pc.
RT Lac     RS CVn, third body, period change (Lac_12, Lac_13, Lac_14); the
RT Lac      variation of orbital period shows a correlation with the activity 
RT Lac      level of the primary component (Lac_5).
UW Lac     Apsidal motion (Lac_15).
AU Lac     Eccentric orbit (Lac_16).
DG Lac     Period change (Lac_3).
Y Leo      HIP d=239(88) pc ; Orbital period is variable and O-C diagram shows
Y Leo       sinusoidal variations (Leo_5,KKN).
UU Leo     Orbital period variation (KKN).
VZ Leo     Orbital period is variable and O-C shows parabolic variations
VZ Leo      (KKN, Leo_6).
T LMi      Orbital period variation (LMi_3, KKN).
RS Lep     Orbital Period Variation (KKN).
Delta Lib  HIP d=93.3(7.9) pc, Apsidal Motion (Lib_3), Orbital period variation 
Delta Lib   (KKN).
RV Lib     HIP d=370(290) pc.
SS Lib     HIP d=330(200) pc, Orbital period variation (KKN).
Beta Lyr   HIP d=270(38) pc; High rate mass transfer:2x10^-5^(M/year) (Lyr_1).
RV Lyr     Orbital period variation (KKN).
TT Lyr     Tycho d=91(66) pc.
EW Lyr     Orbital period variation (KKN).
RW Mon     HIP d=230(81), Orbital period variation (KKN).
TU Mon     HIP d=370(170) pc.
AR Mon     HIP d=276(93) pc.
AU Mon     Circumstellar matter, presumably associated with the accretion disk
AU Mon      (Mon_15).
BO Mon     Orbital period variation (KKN).
V635 Mon   HIP d=330(110) pc.
V745 Mon   HIP d=249(66) pc, It was newly classified by Hipparcos.
UV Mus     Tycho d=27(18) pc.
DZ Mus     HIP d=321(97) pc.
RV Oph     Magnetic activity (Oph_1).
RZ Oph     HIP d= 430(380) pc : Accretion disk (Oph_6).
UU Oph     HIP d= 139(37) pc .
DN Ori     HIP d=390(180) pc, Accretion disk structure around the primary
DN Ori      component (Ori_3).
EQ Ori     Orbital period variation (KKN).
EY Ori     HIP d=420(270) pc.
FH Ori     Orbital period variation (KKN).
FK Ori     Orbital period variation (KKN).
FL Ori     Orbital period variation (KKN).
OS Ori     Orbital period variation (KKN).
TY Peg     HIP d= 230(88) pc.
AQ Peg     HIP d= 490(420) pc.
AW Peg     HIP d=160(24) pc.
DF Peg     HIP d= 470(260) pc.
DI Peg     HIP d=193(64) pc.
Beta Per   HIP d=28.46(0.73) pc ; Third body with mass 1.8 M and mass transfer
Beta Per    (Per_1) ; Asymetric transient accretion disk (Per_11).
Z Per      Decreasing period and irregular period jumps (Per_17).
RT Per     HIP d=180(70) pc; Period decrease and third body (Per_18).
RV Per     Orbital period variation (KKN).
RW Per     HIP d=290(120) pc; Disk structure (Per_8); Orbital period variation 
RW Per      (KKN).
RY Per     HIP d=630(470) pc; The border between permanent and transient disk
RY Per     (Per_3).
ST Per     Orbital period variation (KKN), Third and forth body from orbital
ST Per      period analysis (Per_19).
WY Per     Orbital period variation (KKN).
XZ Per     Orbital period variation (KKN).
DM Per     HIP d=580(320) pc ; Triple system (Per_10).
V436 Per   HIP d=315 pc, Apsidal motion (Per_20).
Y Psc      Orbital period is variable (Psc_4, KKN).
XZ Pup     HIP d=253(66) pc; Orbital period variation (KKN).
V397 Pup   HIP d=147(11) pc, It was newly classified by HIPPARCOS.
U Sge      HIP d=311(71) pc ; Orbital period variability due to apsidal
U Sge       motion (Sge_3) ; It has a accretion disk around primary component
U Sge       (Sge_4).
UZ Sge     Orbital period variation (KKN).
RS Sgr     HIP d=270(63)pc ; Increasing period due to the mass transfer (Sge_3),
RS Sgr      Apsidal Motion (Sgr_8).
SX Sgr     TYCHO d=40(32) pc .
WX Sgr     Orbital period variation (KKN).
XY Sgr     Orbital period variation (KKN).
XZ Sgr     HIP d=234(78) pc; Orbital period variation (KKN).
EG Sgr     Orbital period variation (KKN).
V356 Sgr   HIP d=600(360) pc.
V505 Sgr   HIP d=117(19) pc, Orbital period variation, third body (Sgr_10, KKN).
FV Sco     HIP d=720(480) pc, new classified star, periodic variable; radio
FV Sco      continuum emission (Sco_1); a microwave survey of southern active
FV Sco      stars (Sco_2).
V393 Sco   HIP d=470(260) pc, new classified star, periodic variable; radio
V393 Sco    continuum emission (Sco_1); a microwave survey of southern active
V393 Sco    stars (Sco_2).
U Sct      Orbital period variation (KKN).
RS Sct     HIP d=260(110) pc, Orbital period variation (KKN).
RY Sct     Disk structure (Sct_9), Orbital period variation (Sct_11, KKN).
RZ Sct     HIP d=800(650) pc, Orbital period variation (KKN).
BS Sct     Orbital period variation (KKN).
W Ser      HIP d=370(180) pc, Orbital period variation (KKN).
AK Ser     Orbital period variation (KKN).
AO Ser     Orbital period variation (KKN).
Lamda Tau  HIP d=114 pc: Third body (Tau_9); apsidal motion (Tau_12).
RW Tau     HIP d=300 pc; accertion disk (Tau_13).
AC Tau     Period change, third body (Tau_12).
BN Tau     Orbital period variation (KKN).
HU Tau     HIP d=111(10) pc.
X Tri      HIP d=166(35) pc .
TX UMa     HIP d=211(48) pc ; Apsidal Motion (UMa_9); Accretion Disk Structure
TX UMa     (UMa_10).
VV UMa     O-C shows sinusoidal variation due to the third body (UMa_10).
XZ UMa     Orbital period variation (KKN).
AC UMa     Orbital period variation (KKN).
RW UMa     HIP d=240(110) pc.
W UMi      HIP d=450(150) pc ; Orbital period is variable (UMi_1; KKN).
RU UMi     Large-scale spot activity on the secondary component(UMi_6), Orbital
RU UMi      period variation (KKN).
TY UMi     HIP d=109.9(7.1) pc, It was newly classified by Hipparcos.
S Vel      HIP d=151(18) pc; Orbital period variation (KKN).
RX Vel     TYCHO d=23.8(9.1) pc.
UW Vir     HIP d=460(230) pc; Orbital period variation (KKN).
BD Vir     HIP d=270(100) pc; Orbital period variation (KKN).
DL Vir     HIP d=281(82) pc; Orbital period variation (KKN, Vir_1).
UY Vir     HIP d=132(16) pc.
DM Vir     HIP d=340(150) pc.
Z Vul      HIP d=350(120) pc; Orbital period variation (KKN).
RS Vul     HIP d=287(72) pc.
AX Vul     Orbital period variation (KKN).
AY Vul     Orbital period variation (KKN).
BO Vul     Orbital period variation (KKN).