V0735 And Magnitudes in the Table can be influenced by surrounding bright stars.
V0736 And VB AB (AB 11.03mV; 0.1", 115deg, 1973; A and B estimated equally
V0736 And  bright). Magnitudes in the Table can be influenced by a 10.60mV star
V0736 And  BD +36 0159 (50", 252deg, 1999).
V0744 And Porb=0.02608d.
V0751 And A twice shorter period is not excluded.
V0762 And Studied in [81025] (SAVS 023548+491758) but erroneously identified
V0762 And  with GSC 03303-01008.
CH    Ant Multiperiodic, 4 harmonics. P1 is given in the Table.
CI    Ant VB A (B 13.1m, 1", 306deg, 1991).
CN    Ant P strongly varies. The elements in the Table are for
CN    Ant  JD 2453569 - 2454298.
V0367 Aps VB B (A 11.3m; AB 8", 58deg, 2000).
V0380 Aps VB (several companions).
V0919 Ara SB2.
V0927 Ara VB A (B 13.3m, 14", 121deg, 1999). The magnitude in minimum is
V0927 Ara  influenced with the companion.
V0943 Ara Similarity to FG Sge is not excluded.
V0952 Ara Multiperiodic, 5 frequencies detected.
V0969 Ara VB A (B 13.8m, 16", 148deg, 1999).
V0978 Ara P=46.5d is superposed.
V0981 Ara Blazhko effect, P=58.66d.
V0982 Ara VB B (A 13.9mpg, B 14.3mpg; AB 13", 351deg, 2000).
V0982 Ara  The magnitudes in the Table are influenced by the companion.
CP    Ari VB A (B 7", 149deg, 1997).
CR    Ari Type ELL with the light elements Min=2455181.6141 + 0.361849d x E
CR    Ari  is also possible.
V0674 Aur P=0.29779d is not excluded. Type EW, with periods 0.59563d or
V0674 Aur  0.63533d, is also possible.
V0681 Aur Blazhko effect.
V0695 Aur Running numbers and USNO-B1.0 numbers in [81080] are mixed up;
V0695 Aur  corrected by GCVS compilers.
V0696 Aur Running numbers and USNO-B1.0 numbers in [81080] are mixed up;
V0696 Aur  corrected by GCVS compilers.
V0697 Aur VB A (B 6", 70deg, 1997).
V0698 Aur Eccentric binary. Running numbers and USNO-B1.0 numbers in [81080]
V0698 Aur  are mixed up; corrected by GCVS compilers.
V0707 Aur O'Connell effect.
V0708 Aur O'Connell effect.
V0716 Aur MinII - MinI=0.47P.
V0742 Aur DSCTC type with P=0.132695d is also possible.
V0744 Aur VB A (B 5", 9deg, 2000). P=0.362922d is also possible.
V0746 Aur P=0.086921d is also possible.
V0750 Aur Multiperiodic, P2=0.069397.
V0754 Aur P=0.33285d is also possible.
V0765 Aur VB A (B 4", 91deg, 1997).
V0786 Aur VB A (B 3", 183deg, 1989).
V0790 Aur Type EW with a twice longer period is not excluded.
V0798 Aur VB A (12.4mV; B 14.7:mV, 7", 286deg, 1998).
V0803 Aur Multiperiodic. P2=0.05503008d, P3=0.04250400d.
V0808 Aur Eclipses: Min=2455126.8960 + 0.081376d x E, range 17.8 - 21.4 V,
V0808 Aur  D=0.06P.
V0815 Aur VB A (B 16.5mpg, 5", 75deg, 2000).
V0817 Aur MinII - MinI=0.32P.
V0823 Aur Secondary period P2=0.2980d.
V0349 Boo P strongly varies. The coordinates in [81005] refer to a brighter
V0349 Boo  neighbor.
V0352 Boo Multiperiodic. The period of the first-overtone radial mode is given
V0352 Boo  in the Table. Two non-radial modes: P2=0.347051d, P3=0.342383d.
V0524 Cam Distortion wave: P=0.499464d.
V0525 Cam Distortion wave: P=0.461208d.
V0534 Cam MinII - MinI=0.545P.
V0542 Cam Multiperiodic. P1 is presented in the Table; P0=0.174773d.
V0542 Cam  VB A (11.70mV; B 13.55mV, 17", 191deg, 1999).
V0549 Cam MinII - MinI=0.543P. O'Connell effect.
V0565 Cam VB A (B 14.9mF, 7", 139deg, 2000); the amplitude in the Table is too
V0565 Cam  low because of the companion.
MR    Cnc Pulsates in the first overtone (see Table) and fundamental
MR    Cnc  (Max=2454701.537 + 0.536525d x E) modes. P1/P0=0.7462.
MY    Cnc Double-mode, with a radial and a none-radial modes excited. The second
MY    Cnc  light elements: Max=2454700.652 + 0.281995d x E. P2/P1=0.9824.
GP    CVn Light elements for eclipses: Min=2453796.248245 + 0.062959041d x E
GP    CVn  [81139].
GR    CVn The Table presents the period of first-overtone pulsations;
GR    CVn  P0=0.486651d. P1/P0=0.7443.
V0432 CMa MinII - MinI=0.53P.
V0835 Car SB2.
V0845 Car SB2.
V0846 Car Multiperiodic, 3 harmonics.
V0865 Car MinII - MinI=0.605P.
V0867 Car VB B (A 12.6mV; AB 4.5", 194deg, 2000).
V0869 Car MinII - MinI=0.45P.
V0887 Car MinII - MinI=0.445P.
V0889 Car MinII - MinI=0.370P.
V0890 Car A twice shorter period is also possible.
V0899 Car Double-mode pulsations. The Table gives the fundamental-mode elements.
V0899 Car  For the first overtone, P1=0.0858512d.  P1/P0=0.7748.
V0901 Car Large scatter outside eclipses; intrinsic variability?
V1255 Cas Twice shorter period and type RRC are possible.
V1271 Cas MinII - MinI=0.525P.
V1276 Cas Light curve shape varies.
V1277 Cas Multiperiodic, P2=0.0876987d.
V1280 Cas Multiperiodic.
V1375 Cen Porb=0.3604d? [81150].
V1389 Cen SB2?
V1393 Cen Double-mode pulsations. P1 is given in the Table. P0=0.1177831.
V1393 Cen  P1/P0=0.7712.
V1397 Cen Blazhko effect, P=146d.
V1400 Cen Starspots rotational modulation with P=3.219d. One deep minimum, with
V1400 Cen  secondary fadings before and after it, was observed.
V1400 Cen  Probably a pre-main sequence star.
IO    Cet VB A (12.1mV; B 13mV, 14", 173deg, 1998). The range in the Table
IO    Cet  is for combined magnitudes.
IQ    Cet P1 is presented in the Table; P1/P0=0.7438.
IU    Cet P1 is presented in the Table; P1/P0=0.7425.
IZ    Cet SB, Porb=8.1194d.
KM    Cet P1 is presented in the Table. P0=0.542695d.
KN    Cet Eclipsing variability outside outbursts: 17.2m*-19.9m*,
KN    Cet  Min=2455202.5579 + 0.05298466 x E [81196].
KR    Cet P1 is presented in the Table; P1/P0=0.7434.
FG    Cir VB A (B 13.9mpg, 19", 339deg, 2000); B is in 3" sf to AR Cir,
FG    Cir  Nova Cir 1906.
FH    Cir Multiperiodic. Light elements with P1 are given in the Table.
FH    Cir  P2=0.1260864. P2/P1=0.8279.
BI    Col Type EW with a twice longer period is not excluded, having in mind
BI    Col  association with an X-ray source [81001].
BK    Col P varies strongly [80001].
BL    Col Blazhko effect, P=40.5d.
BQ    Col Blazhko effect, P=15.33d?
QQ    Com P strongly varies.
CZ    CrB P strongly varies.
YZ    Crv VB B (A 16.2mpg, B 16.2mpg; AB 27", 192deg, 2000).
YZ    Crv  The coordinates in [81005] refer to the A component.
AA    Crv VB B (A 12.7mpg, B 15.9mpg; AB 28", 220deg, 1998).
AA    Crv  The coordinates in [81005] refer to the brighter star.
V0458 Dra The light elements could not be confirmed [81001] using the Catalina
V0458 Dra  Surveys data.
V0462 Dra P=0.21157d is not excluded.
V0472 Dra VB B (A 13.7m; B 14.5m, 19", 199deg, 1999).
V0472 Dra  The tabulated variability range is influenced with the companion.
V0485 Dra Type ELL is not excluded.
V0486 Dra The coordinates in [81005] refer to a neighbor star.
V0506 Dra P varies.
NN    Eri Blazhko effect, P=335.29d.
NP    Eri Blazhko effect [81005].
NX    Eri P0 is presented in the Table; P1=0.354824d.
BF    For VB A (B 11.0m, 2", 170deg, 1991).
BI    For P varies? Light elements for JD 2454000 - 2455165 are presented in
BI    For  the Table.
V0439 Gem A twice longer period is not excluded.
V0455 Gem Multiperiodic.
V1366 Her P strongly varies, current elements after JD 2456000 are given in
V1366 Her  the Table.
V1373 Her Period varies.
V1377 Her Period varies.
V1390 Her MinII - MinI=0.46P.
V1396 Her Blazhko effect.
V0571 Hya Blazhko effect, P=11.80d.
V0575 Hya Blazhko effect, P=8.52d.
V0588 Hya Blazhko effect, P=87.73d [81056].
V0592 Hya Possibly Blazhko effect with P=14.2d.
V0598 Hya VB A (15.4mpg; B 15.6mpg, 18", 43deg, 2000).
V0598 Hya  The coordinates in [81005] refer to the companion.
V0599 Hya VB B (A 15.1mpg, B 16.6mpg; AB 29", 152deg, 2000).
V0599 Hya  The coordinates in [81005] refer to the brighter star.
V0603 Hya Double-mode pulsations. The Table contains the period for the first
V0603 Hya  overtone. Fundamental mode: P0=0.4867803. P1/P0=0.7449.
LR    Leo Pulsates in the first overtone (see Table) and fundamental
LR    Leo  (Max=2454701.577 + 0.557447d x E) modes. P1/P0=0.7469.
LR    Leo  A nonradial mode with P=0.559369d may also be present.
LU    Leo O'Connell effect.
LY    Leo O'Connell effect.
LZ    Leo VB A (13.6mV; B 15.7mV, 9", 258deg, 2000).
MV    Leo Porb=0.14608d.
NV    Leo Double-mode pulsations. The Table gives the first-overtone light
NV    Leo  elements. For the fundamental mode,
NV    Leo  Max=2454800.541 + 0.483098d x E. P1/P0=0.7441.
OX    Leo Multiperiodic. P2=0.89405d.
BL    Lep VB (6", 19deg, 1999); the variable is probably the southern component.
BL    Lep  Combined magnitudes are presented in the Table.
BN    Lep P varies strongly.
BO    Lep VB A (11.4mV; B 11.6mV, 19", 163deg, 1998).
V0364 Lib Two outbursts were observed. Porb=0.70242d.
V0366 Lib P varies. The light elements in the Table are for JD 2453639-2455100.
V0368 Lib Double-mode pulsations. The Table contains light elements for the
V0368 Lib  first overtone. Fundamental mode: Max=2455000.800 + 0.57857d x E.
V0368 Lib  P1/P0=0.7443.
HS    Lyn A twice shorter period is not excluded.
IW    Lyn VB A (B 7", 349deg, 1999).
IZ    Lyn Probably a VB unresolved in the photometry.
KX    Lyn [Fe/H]=-1.9.
LO    Lyn Blazhko effect, P=9.763d.
LR    Lyn Blazhko effect? [81001].
V0960 Mon In a nebula.
V0962 Mon SB2, Porb=5.32d; the F2V component varies. Multiperiodic;
V0962 Mon  other periods are P2=0.77214d and P3=0.68432d.
V0964 Mon VB AB (12.5m, 13.0m, 2".7, 213deg, 2000).
V0965 Mon Blazhko effect, P=37.24d.
V0966 Mon Pulsates in the first (see Table) and second
V0966 Mon  (Max=2453761.54 + 0.85905d x E) overtone modes. P2/P1=0.8043.
V0972 Mon A period of 0.948d was also detected.
V0973 Mon The amplitude of periodic variations (see Table) is 0.08m;
V0973 Mon  a single flare was observed.
V0975 Mon Light elements for eclipses are tabulated. Outside eclipses, P=3.25d,
V0975 Mon  amplitude 0.03m. VB A (B=NSV 03138, 16.1-16.7mV, 7", 357deg, 1999).
V0979 Mon The light elements for the first overtone are given in the Table.
V0979 Mon  Second overtone: Max=2453800.32 + 1.03153 x E. P2/P1=0.8005.
V0982 Mon VB A (B 14.35mF, 10", 256deg, 1998).
V0985 Mon Pulsates in the first (see Table) and second
V0985 Mon  (Max=2453674.01 + 0.70772d x E) overtone modes. P2/P1=0.8046.
V0988 Mon P=0.36319d is also possible.
V0989 Mon VB A (B 6", 264deg, 1998).
V0355 Mus SB2.
V0356 Mus Double-mode pulsations. The Table gives the first-overtone light
V0356 Mus  elements. For the second overtone,
V0356 Mus  Max=2453693.12 + 0.734376d x E. P2/P1=0.8043.
V0495 Nor SB2.
V0498 Nor VB B (A 9.25mV; B 9.72mV, A6V, 7", 160deg, 1998).
V0498 Nor  Combined magnitudes are presented in the Table.
V0501 Nor VB A (B 5", 99deg, 20000). Combined magnitudes are presented in
V0501 Nor  the Table.
V2837 Oph The period in the Table is that of spot variability. SB2, Porb=591d.
V2837 Oph  VB A (B=V2252 Oph, 13", 123deg, 1998).
V2857 Oph O'Connell effect.
V2862 Oph VB A (B 19.7m, 2.5", 289deg).
V2897 Oph P=129d is superposed.
V2918 Oph A twice shorter period is not excluded.
V2925 Oph P varies [81101].
V2930 Oph Blazhko effect.
V2947 Oph VB A (B 14.0m, 12", 93deg, 1998). The magnitude at minimum in the
V2947 Oph  Table can be influenced by the companion.
V2797 Ori Multiperiodic.
V0966 Per MinII - MinI=0.33P. e=0.284.
V0982 Per MinII - MinI=0.38P.
V1024 Per VB A (B 4", 168deg, 1989).
V1035 Per Type DSCT with P=0.1441d is also possible.
V1036 Per Type SR with P=71d is not excluded.
V1041 Per Type SR with P=160d is not excluded.
V1043 Per The epoch in the Table corresponds to the eclipse-like feature of the
V1043 Per  light curve but not to the overall brightness minimum.
DN    Phe Blazhko effect?
DP    Phe P probably varies.
DR    Phe Blazhko effect, P=40.17d [81056].
AW    Pic Blazhko effect. P(Bl)=756d [81001].
AX    Pic P varies.
AY    Pic SB2.
V0707 Pup P varies strongly.
V0711 Pup VB A (B 5", 128deg, 1999).
V0714 Pup Blazhko effect, P=116.96d.
V0716 Pup P varies strongly.
V0719 Pup Pulsates in the first (see Table) and second
V0719 Pup  (Max=2453455.40 + 0.593216d x E) overtone modes. P2/P1=0.8057.
V0719 Pup  VB A (B 11.0m, 6", 42deg, 1999); the tabulated range is for the
V0719 Pup  combined brightness.
V0722 Pup SB2.
V0725 Pup VB A (B 10.3m, 1", 47deg, 1991).
V0732 Pup Pulsates in the first (see Table) and second
V0732 Pup  (Max=2453456.065 + 0.333105d x E) overtone modes. P2/P1=0.8007.
V0733 Pup Pulsates in the fundamental mode (see Table) and in the first overtone
V0733 Pup  (Max=2453600.055 + 0.1742342d x E). P1/P0=0.7618.
V1537 Sco Multiperiodic. VB A (8.1mV; B 12.6mV, 1.9", 231deg, 1939).
V1544 Sco It is assumed that there is a typo in the star's declination
V1544 Sco  in [81021].
V1547 Sco Simultaneous presence of two periods. P1 is given in the Table.
V1547 Sco  P2=2.27816d.
V1552 Sco VB A (B 16.0m, 11", 111deg, 2000).
V1553 Sco Double-mode pulsations. The period for the fundamental mode is given
V1553 Sco  in the Table. P1=0.1470447d. P1/P0=0.7978.
V1560 Sco VB A (B 15.0m, 6", 147deg, 1999).
V1611 Sco MinII - MinI=0.65P.
V1614 Sco Several close companions.
CY    Scl Blazhko effect.
DE    Scl P1 is presented in the Table; P1/P0=0.7448.
DI    Scl SB2.
V0562 Ser d=0.07P.
V0575 Ser Double-mode pulsations. The Table contains light elements for the
V0575 Ser  first overtone. Fundamental mode: Max=2454700.867 + 0.475615d x E.
V0575 Ser  P1/P0=0.7446.
V0579 Ser Double-mode pulsations. The Table contains light elements for the
V0579 Ser  first overtone. Fundamental mode: Max=2454800.609 + 0.479144d x E.
V0579 Ser  P1/P0=0.7444.
V0585 Ser SiO maser.
V0592 Ser VB A (B 14.0mpg, 13", 80deg, 1998).
V0595 Ser VB A (B 5" p).
BY    Sex Pulsates in the first overtone (see Table) and fundamental
BY    Sex  (Max=2454801.000 + 0.581288d x E) modes. P1/P0=0.7473.
CF    Sex P strongly varies. The elements in the Table are for
CF    Sex  JD 2455900-2456500.
V1384 Tau Multiperiodic. P1 is presented in the Table; P0=0.1397914d.
V1392 Tau Multiperiodic. P0 is presented in the Table; P1=0.0579031d.
V1403 Tau Close VB.
V1412 Tau P=0.3409505d is also possible.
V1414 Tau P=0.195018d is also possible.
DE    Tri P=30.6d is not excluded.
V0347 TrA Blazhko effect, P=118.05d.
V0348 TrA Double-mode pulsations. The Table contains light elements for the
V0348 TrA  first overtone. Second overtone: Max=2453600.091 + 0.1224057d x E.
V0348 TrA  P2/P1=0.8279.
V0351 TrA P=49.5d is superposed.
V0374 UMa Multiperiodic, 4 harmonics.
V0379 UMa P1 is given in the Table. P0=0.494909d, P1/P0=0.7446.
V0380 UMa Pulsates in the first overtone (see Table) and fundamental
V0380 UMa  (Max=2454876.9243 + 0.47451d x E) modes. P1/P0=0.743.
V0384 UMa Type EW with a twice longer period is also possible.
V0389 UMa Double-mode pulsations. The Table gives the first-overtone light
V0389 UMa  elements. For the fundamental mode,
V0389 UMa  Max=2454847.9552 + 0.47119d x E. P1/P0=0.744.
V0415 UMa P=1.56575d is also possible.
V0417 UMa O'Connell effect.
V0430 UMa Other detected periods are 0.0037005d and 0.0024173d.
AN    UMi VB A (14.4mV; B 15.8mV, 8", 63deg, 2000). The variability range in
AN    UMi  the Table is for combined light.
V0519 Vel Pulsates in the first (see Table) and second
V0519 Vel  (Max=2453426.48 + 0.939354d x E) overtone modes. P2/P1=0.8052.
V0526 Vel Double-mode pulsation. For the fundamental-mode period, see the Table.
V0526 Vel  P1=0.0624889d, P1/P0=0.8062.
V0528 Vel Multiperiodic, 4 harmonics.
V0533 Vel SB2.
V0540 Vel Double-mode pulsation. P2=0.1765777d.
V0547 Vel SB2.
V0548 Vel Multiperiodic. P2=0.0482189d.
V0613 Vir P strongly varies.
V0630 Vir The Table presents the light elements for the first overtone. For the
V0630 Vir  fundamental mode, Max=2454800.650 + 0.524429d x E. P1/P0=0.7453.
V0644 Vir Double-mode pulsations. The Table gives the first overtone light
V0644 Vir  elements. For the fundamental mode, Max=2454800.145 + 0.455977d x E.
V0644 Vir  P1/P0=0.7426.
V0659 Vir Double-mode pulsations. The Table contains light elements for the
V0659 Vir  first overtone. Fundamental mode: Max=2454800.750 + 0.505828d x E.
V0659 Vir  P1/P0=0.7450.