| Name --- | Text --- |
|---|---|
| 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). |