Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.sai.msu.su/gcvs/gcvs/vol1/rem.txt Дата изменения: Mon Apr 7 18:32:44 2003 Дата индексирования: Sat Dec 22 06:34:56 2007 Кодировка: Поисковые слова: принцип мопертюи

R And S5/4.5e.
S And SN (NGC 224).
W And S7.5/1-e.
X And S5/7-e.
Z And The light curve is characterized
by outbursts up to 4m with intervals of 10 - 20
years. In the intervals cyclic variations are observed with
the mean period of 632d and variations with cycles of
several days and Delta(m) ~ 0.1m - 0.5m. The spectrum is
symbiotic, with features of a late M giant, narrow
low-excitation emission lines (Bleq) and forbidden lines
characteristic of highly excited nebulae.
RR And S6/3.5e.
RT And Min II 8.88; DI = DII = 0.17P; dI = dII = 0.00. P var.
Nonlinear term: -6.33*10**(-11)*E**2. During
JD2433477 - 43878 linear elements are satisfactory:
Min = 2441141.8888 + 0.62892984d*E. Period changes
according to a sine law are possible [08002].
RU And P var. Max = 2419857 + 243.0d*E (JD2412800 -
20000); Max = 2434551 + 233.24d*E (JD2420000 -
34550). Since JD2435000 - see Table. Delta(m) ~ 4m - 5m
(before JD2429600), ~1m (JD2429600 ~ 33600), up to 3m
(JD ~2436000), ~1.5m (JD ~2436700). In 1970 - 1972
showed quite irregular variations.
RX And SB (P = 0.21173d). Cyclic variations with P ~ 38s - 54s
were observed after a normal maximum; after a short
maximum no periodicity was found [08004].
SS And Two long period variations are also observed:
P = 650d, P = 3800d.
ST And P var. Max = 2418370 + 337.3d*E (JD2418000 - 28000).
Since JD2428000 - see Table.
SU And VB A (B 12.77m V, F0V:, 15").
SV And The magnitude in Max varies periodically, P = 930d,
P = 5400d? [02146].
SW And [Fe/H] = +0.16. P var. Nonlinear term:
-1.229d*10**(-10)*E**2 [01959]. Since 1959
Max = 2436466.828 + 0.442270121d*E [06929].
The shape of the light curve varies with
Pi ~36.83d = 83.28 P. The deviations (O - C) satisfy
the elements of Blazhko effect
Max(O - C) = 2436816.23 + 36.921d*N. Secular trend
and cyclic (P ~2a) variations of (O - C) are possible
[08005].
SY And d = 0.027P.
TT And Min II 11.6?
TU And P var (Pi ~37a?).
TV And P var? Delta(m) strongly varies.
TW And d = 0.020P. Min II 8.94. P var. Min = 2428845.422 +
4.122739d*E (JD2420050 - 32000). Since JD2432000 - see
Table.
TZ And P1 = 118d: [00882].
Mean magnitude varies with P2 = 974d [00098]. P = 135d
(JD2437545 - 38377) [03367].
UU And P var. Min = 2428832.536 + 1.486311d*E (JD2421455 - 23740)
[02262]; Min = 2428832.465 + 1.48629d*E (JD2428830 - 35012)
[00745]. Since JD2441100 - see Table.
UW And P var. Before JD2430000 Max = 2418585 + 236.7d*E. Since
JD2436000 - see Table.
WW And d = 0.012P.
WX And P var. Max = 2422613.614 + 3.0012544d*E (JD2422610 - 34712)
[01240]. The Table gives current elements. d = 0.03P
in 1972 and probably varies.
WZ And Min II 11.9. P var [02262]. Min = 2435075.342 + 0.695662d*E
(before JD2440500); probably
Min = 2440872.290 + 0.6956576d*E since JD2440500.
The elements in the Table represent all the observations
satisfactorily.
XX And P var. Max = 2418001.938 + 0.7227486d*E (1908 - 1932);
Max = 2427106.403 + 0.7227591d*E (1932 - 1946) [02264].
Since 1946 - see Table. Delta(S) = 9. Blazhko effect:
Max = 2437578 + 36d*N [03111].
XY And Blazhko effect is possible.
XZ And Min II 10.16; DII = 0.26P. P var [02431, 06932, 08008,
08593]. Min = 2432883.6046 + 1.3572708d*E (JD2431700 -
36150) [01977]; Min = 2441954.340 + 1.357293d*E
(since JD2436200). The elements in the Table represent all
the observations satisfactorily.
AA And Min II 10.5.
AB And Min II 10.20. P var. Period increased suddenly in 1953
( ~JD2434500); no period changes later [02509, 05222].
Elements since 1953 - see Table.
AC And Unusual multiperiodical variable. Second oscillation:
Max = 2432467.373 + 0.71124243d*E; P3 = 0.421069d [08187],
see also [08294, 08295]. Delta(S) = -1:.
AD And Min II 11.6. Depth of minima in yellow light: 0.62m (Min I),
0.58m (Min II) [03141]. Min II - Min I = 0.494P. P var.
Min = 2428718.402 + 0.9861940d*E (JD2417460 - 29640)
[01983]. Since JD2428700 - see Table.
AE And In the M31 galaxy. Strong UV continuum.
Emissions: H, He I, Fe II, [Fe II].
AF And In the M31 galaxy. Strong UV continuum.
Emissions: H, He I, Fe II, [Fe II].
AG And According to [08296], DSCT:, Min = 2442636.5868 + 0.0347d*E,
A = 0.5m.
AM And VB A (B 0.25' S).
AN And Min II 6.09. The existence of the third body in
the system is possible. Sp(Met) = F2 - F5.
AP And Min II 11.9. The period may be 2 times shorter.
AT And B - V: +0.42, +0.56. Delta(S) = 3. See [08299] for data
on period variations and a detailed study.
BD And Min II 11.4.
BE And Average cycle: 137d [01993, 02267]; 156.8d after JD2431700.
BL And Depth of Min II 0.24m: P var? Min I = 2429491.255 +
0.7223779d*E (JD2415800 - 33900) [01995]. Since JD2433900 -
see Table.
BX And ADS 1671 A (B 9.7m, 20", 59deg). Min II 9.15. Possible
period change from 0.61011222d to 0.61011534d (~1952).
On the period changes see also [08657].
BY And According to [08658], SRB:.
CC And Possibly in a binary with Porb = 10.469d. Delta(m) and the
light curve shape vary with a period 5.23714d or 10.469d
[08016]. According to [03120], 4 periods are present:
P2 = 0.0632083d. First overtone was not found. Other
periods are resonances.
CG And P var: 3.7430d (1950), 3.7394d (1963) [05224].
Cyclic period changes are possible.
According to [06941], short period oscillations (P = 2h 04m)
are present. A number of observers do not find short-term
variability.
CM And According to [00821], Max = 2428380 + 140d*E and Max =
2430616 + 124d*E, and the star resembles UU Her.
CN And Min II 9.96.
CO And d = 0.06P:
CP And d = 0.01P? Depth of Min II 0.05m?
CU And d > 0.034P ([06943], according to visual observations.)
DI And DCEP? [03165].
DK And EW?
DL And In the field of the open cluster NGC 7686.
DR And P var. Before ~JD2437000 Max = 2436078.384 + 0.5630609d*E
[02275]; then P changed abruptly. Delta(m) changes by ~0.3m,
Max A1 = 2436078.8 + 69.486d*N1, Max A2 = 2437646.65 +
69.719d*N2. Other possible cycles are 2000d (interaction
of cycles N1 and N2) and ~30 years [08019].
DS And In the field of the open cluster NGC 752. Min II 10.7.
DZ And According to [04008], type RCB, spectrum R. According to
[06945], since 1961 is in Max light all the time. According
to [06946], the spectrum is not characteristic of RCB stars.
According to [08660], the star was bright near the moments
of Min light given in [04008].
EG And P = 40d or 80d [08020].
Absorption spectrum with overlaying emissions of high
excitation [04434, 08598]. Strong variable magnetic field
[04435]. Long period variations of light are observed.
Radial velocities profiles and equivalent widths of lines
vary with P = 470d [08596] (SB? [08597]). Possibly is
analogous to HM Sge [08598].
EH And IR excess. The presence of a dust envelope is possible.
EO And Very red.
EP And Min II 12.5.
ET And Delta(B) = 0.035m, Delta(U) = 0.07m.
The Table gives the epoch of Max light. Observations may
be represented by the periods 0.723d and 1.61553d
[08022, 07946]. According to [08023], in June - December 1977
Min = 2443337.4725 + 0.49925d*E, other periods are
not satisfied by observations. According to [08599],
Max(U) = 2439751.28 + 0.617135d*E (1967 - 1971).
SB, Max(Vr) = JD2443718.0 + 48.304d*E [08301].
Photometric periods could not be found in radial
velocities.
EX And Possible Min II 13.0:, Min II - Min I = 0.55P.
EY And I - K = 5.38;
the presence of a dust envelope is possible [06947].
FF And 10.35m - 10.42m V outside flares; M - m = 0.50P.
Porb = 2.170304d [08024]. According to photometric
observations, P = 2.14d (1971), P = 2.15d (1972),
P = 2.19d (1973) [06948].
FG And According to [04156], EA; Min = 2436074.528 + 0.99772d*E.
FL And d = 0.02P.
FZ And mu = 1", p = 64deg.
GK And Min II 11.5.
GN And ADS 409 A (B 13.3m, 2", 6deg; C 11.6m, 141", 130deg).
Different authors give spectral types F0 III, F2V, Am
(probably based on different criteria).
GP And Delta(m) changes with P2 = 0.64d.
A wave with P3 = 0.012161d is present. The mean
magnitude and the shape of the light curve vary
[08302].
GQ And ADS 246 B (A = GX And; B 37", 61deg). B - V = +1.80.
X-ray source.
GR And Min (magnet.field) = 2442288 + 525d*E.
Magnetic field varies (-250 to -1030 Gauss). Period of
changes of C1 is near 1.5 years [07893]. According to [06257],
period of changes in u is near 1 year or longer.
GS And B - V = +1.7 in normal light.
GX And ADS 246 A (B = GQ And, 37", 61deg). Delta(U) = 0.55m. SB?
(conflicting data).
GY And SB1 (P = 273.2d [07324], P = 272.99d [08303]).
For spectral changes, variations of light and magnetic
field it is possible that P = 23a [07004] or 20.60a [08303].
[08022] gives P ~36.5d and Delta(V) ~0.049m. Periods 4.92a
and 1.8d may exist [08303].
GZ And B - V: +0.77, +0.82. ADS 1693 A (B 11.13m, 8", 31deg).
Min II 11.58. P var?
The period is based only on Minima I [06830] and
was improved with account of recent data.
HH And Subdwarf? [06581]. mu = 1.82", p = 176deg.
HI And B - V = 1.8m outside flares.
HN And Max(U) = 2438327.8 + 69.433d*E [08022]. SB
(P = 106.27d [07435]).
HQ And According to [08659], a probable cataclysmic binary;
similarity to AM Her and AN UMa is noted.
HR And d = 0.05P.
HT And B - V = +0.60. In the region of M 31.
HU And Min II 17.2. In the region of M 31.
HV And According to [08659], a probable cataclysmic binary;
similarity to AM Her and AN UMa is noted.
HY And In the region of M 31.
HZ And In the region of M 31. P > 100d. Red.
IL And d = 0.02P.
IM And In the region of M 31.8.
IO And According to [08659], a probable cataclysmic binary;
similarity to AM Her and AN UMa is noted.
IP And d = 0.02P:.
KK And The light curve has double-wave shape
[07740]. Long period variations were found [07955].
KU And I - K = 4.63.
SR type is possible. Surrounded with a dust envelope [08029].
KX And SB2 (P = 38.908d).
KZ And ADS 16557 B (A 7.0m; B 15", 254).
LM And Min II 12.7.
LN And Delta(B) = 0.025.
LO And Min II 11.82.
V0369 And VB (0".1, 128 deg, 1986.9).
V0374 And Not identical with BD+44 422.
alf And SB (P = 96.6960d). VB A (B 11.2m, 80").
Epoch of Max U light is given.
Hbeta index varies in the range of ~0.02m with P
~3h [08030]. Rapid rotation.
zet And Depth of Min II 0.1m. SB.
Unstable light curve. Most notable
variations on the rising branch of Max II [08030].
Many peculiarities in the spectrum.
lam And SB1 (P = 20.52d).
omi And v sin i = 300 km/s; VB(0.3"; possibly
also 0.05" - according to speckle-interferometric data).
Shell spectrum appeared and disappeared several
times since 1890. Different authors attributed
the star to EB type. According to [05955], The changes
of light may be explained also by intrinsic
variations of a single shell star. They are represented
by elements: Min I = 2439470.628 + 1.0185d*E.
According to [02572], Min I = 2436174.430 +
1.5998398d*E. The periodogram analysis shows
a stable peak at P ~0.84d [08032]. A possible shell
event was observed late in 1975.
S Ant Min II 6.87. P var?
T Ant CWB? P var. [A/H] = -0.0. P = 5.9098d (JD2428187 -
34688), P = 5.8976d (JD2434688 - 37660) [05387].
The Table gives mean elements which satisfy all
observations well enough.
V Ant OH, H2O maser.
Z Ant Mean brightness varies with P = 1143d.
SW Ant Min II 14.6.
UZ Ant P var?
WY Ant P var. P = 0.57430871d (JD2414000 - 22070); P =
0.57431618d (JD2422070 - 25600); P = 0.57431216d
(JD2425600 - 29000) [01113]. (k - b)2 = 0.00.
WZ Ant Min II 11.8.
XX Ant Min II 9.1.
XY Ant Depth of Min II 0.3m - 0.5m pg.
XZ Ant Min II 10.2.
Z Aps Possibly also an eclipsing binary.
RT Aps Strong variations of period and the shape of
the light curve [06152].
TY Aps Delta(S) = 3.
YY Aps The period is probably long.
AF Aps Min II 13.9.
AN Aps Min II 12.8.
AP Aps Min II 15.5.
AS Aps Min II 13.8.
AV Aps Depth of Min II 0.05m.
CE Aps P = 209d or 261d.
CY Aps Min II 13.0.
EF Aps Min II 12.6.
FY Aps Deep Min II.
GK Aps Min II 13.9. RRC type is possible.
GO Aps Min II 14.8. RR type is possible.
GQ Aps Min II 14.8.
GU Aps Min II 14.5.
GX Aps RV type is not excluded. The epoch of Min is given.
GY Aps Min II 14.2.
HL Aps Min II 12.6.
HO Aps Min II 13.7.
HT Aps Min II 14.3.
HV Aps Epoch of Min is given.
HX Aps Min II 14.4.
II Aps Min II 11.6.
IL Aps Epoch of Min is given.
IO Aps Min II 12.4.
IR Aps Min II 13.8.
IU Aps Min II 14.6.
IY Aps Min II 12.9.
KN Aps d ~0.03P.
KR Aps Possibly a slow eclipsing variable.
KT Aps Min II 15.2.
KV Aps Min II 13.6.
KZ Aps Smooth light
changes with superimposed variations of eclipsing
nature, with minima on JD2436729 and 2436808.
LM Aps RV type is possible.
LN Aps Min II 13.3.
LO Aps Min II 11.5.
MY Aps L19-2. P0 = 192.75s, P1 = 113.77s.
del 1 Aps In a wide pair (delta2 Aps, 100", common mu).
kap 1 Aps SB? VB A (B 11.27m V, 27").
R Aqr Symbiotic spectrum. Emissions of H, SII, OIII, FeII, NeIII,
OII. Variable radio source. SiO maser. The secondary may
be an accreting white dwarf. The star is embedded in an
expanding gaseous nebula several hundred years
old. A cycle ~24a and longer-term variations are
possible in the changes of radial velocities and period.
U Aqr Strong bands of 12C2, CN,
lines of SrII, YII in the spectrum; hydrogen deficiency.
A probable halo star (Vr ~100 km/s.).
Z Aqr 1969 - 70: P = 100d +- [05973].
RY Aqr P var. Min = 2433872.352 + 1.966598d*E (before
JD2428000); Min = 2440824.410 + 1.966620d*E
(JD2428000 - 41000); Min = 2440824.410 +
1.966611d*E (JD2441000 - 43800). Since
JD2443800 P = 1.966554d?
The Table gives elements representing
observations after JD2428000 with the accuracy +-0.1d.
ST Aqr Min II 9.37. P var. Min = 2423640.271 + 0.78101367d*E
(JD2423500 - 26000) [02037]. Since JD2439700 - see Table.
SU Aqr ADS 16318 A (B 10.7m, 5", 144deg). Min II 10.5. P var?
SV Aqr Cycle 200 - 300d is possible.
SW Aqr P var. (k - b)2 = 0.01.
SX Aqr P var? Delta(S) = 9.
SZ Aqr Epoch of Min is given.
TT Aqr VB A (B 15m, 3", 135deg).
TZ Aqr Delta(S) = 5.
VY Aqr Second outburst: Max ~JD2437897
(1962), ~9m pg [03129].
WX Aqr Blazhko effect is possible.
XZ Aqr P var. Before JD2437913 P = 2.059187d.
YZ Aqr B - V = 0.49 (in Min). (k - b)2 = 0.06.
Small fluctuations of period are possible.
AE Aqr Unusual flare X-ray system with pulsar. Becomes bluer
in Max. In Min B - V = +0.92. Shows rapid irregular
variations, which differ it from UV stars and UG
system, though the spectra are somewhat similar.
Simultaneous photoelectric and spectroscopic observations
[03131] show the existence of two types of flares:
1) intensification of emission lines accompanied by
brightening in U and B; 2) intensification of continuum
leading to brightening in U, B and V ("white flare").
Detailed spectroscopic investigation [01971].
Porb = 0.41165794d + 1.12*10**(-10)*E, The epoch
T0 = JD2439030.621 [08672]. In the X-ray band
(0.1 - 4.0 keV) pulsations with P = 33.0767s are observed
[08673]. In the optical range pulsations with
P0 = 33.076737s as well as with P1 = 16.5s were noted
[08674, 08675].
AT Aqr Min II 14.7.
AX Aqr P var. Before ~JD2427367 Max = 2425417.60 + 0.388135d*E
[03113].
AY Aqr Min II 14.3.
BH Aqr P var. Before ~JD2431150 Max = 2426948.411 + 0.5258022d*E
[03113].
BI Aqr Min II 13.1.
BK Aqr Close companion.
BL Aqr Waves from 80 to 125d. Mean magnitude changes
with cycles from 480 to 700d in the range of 0.3m - 0.6m.
BM Aqr The mean magnitude may vary with P = 500 - 600d.
BN Aqr Delta(S) = 4:. P var. Before JD2428964 Max =
2426577.901 + 0.46963401d*E [03113].
According to [05391] Max = 2429395.742 +
0.4696410d*E + 3.3*10**(-10)*E**2 (1898 - 1958).
BO Aqr P var? (k - b)2 = 0.01.
BQ Aqr d = 0.07P.
BR Aqr P var? (k - b)2 = 0.16.
BS Aqr Delta(S) = 0. P var?
BT Aqr B - V: +0.14, +0.52. P var. Blazhko effect.
BV Aqr P var. Blazhko effect with Pi = 11.56d and variations of
light in Max up to 0.75A.
BW Aqr d = 0.01P. Min II 10.8. Min II - Min I = 0.484P.
Jensch [00189] considers the secondary Min to be the
main one.
BX Aqr d = 0.027P.
CD Aqr d = 0.012P. Min II 10.2.
CE Aqr According to [02548], no
variations were found in visual observations during
several months in 1954 - 1958. According to [03138],
the star may be analogous to AI Vel; P = 0.16d?
CH Aqr P var?
CI Aqr Period may be twice as long.
CM Aqr Min II 13.6.
CP Aqr Delta(S) = 3.
CR Aqr Min II 14.2.
CV Aqr Minor planet (52) Europa.
CW Aqr Min II 10.8.
CX Aqr Min II 10.8. Broad hydrogen lines.
CY Aqr Delta(S) = 2. P var; abrupt change ~1952. Before JD2434000
Max = 2434308.4314 + 0.061038509d*E. The shape of
the light curve probably varies. For M - m different
authors give values from 0.23p to 0.40p. Beat phenomenon
with P2 = 0.2182d is possible [08060].
CZ Aqr Min II 11.1. Cyclic variations of period?
DD Aqr Min II 11.2.
DN Aqr (k - b)2 = 0.01.
DO Aqr P var.
DS Aqr P var.
DV Aqr Min II 6.1. SB. In [08061] variations were noted
with Delta(m) ~0.1m and P < 3h, presumably of DSCT
type nature. Some sources give A3 for the spectral
type. Shell spectrum was observed in May, 1975.
Spectral lines were filled with emission and therefore
weak, strong absorption in H and K CaII lines was present.
Shell effects were not present in the spectra taken in
1971 - 1973 [08062].
DX Aqr VB B (A 7.0m, K0III; B 3.7", 244deg). SB1. d ~0.015P.
Depth of Min II ~0.3m.
The range of combined brightness is given.
DY Aqr d = 0.04P.
EE Aqr Min II 8.48.
EK Aqr Min II 11.23.
EL Aqr P = 0.6345d is possible.
EM Aqr According to [06204] P = 0.068d.
Period and amplitude vary on very short time
scale. Light and colour vary approximately in phase.
The beat period, if exists, is shorter than 1d.
ET Aqr Period is given according to [08336].
EW Aqr Delta(m) varies.
FF Aqr d = 0.059P. SB1. The unique eclipsing system of a red
star and probably a blue hot subdwarf. The amplitude of
the eclipse is 0.15V, 0.4B, 1.2U. The magnitude in Max
varies by 0.35V, 0.33B, 0.22U. Variable shape of light
curve. Strong emissions H and K CaII, Halpha in the
spectrum.
FI Aqr Possibly P = 4.659d or 4.719d. Epoch of min is given.
FK Aqr BDS 11854 A (B = FL Aqr, 11.45m, 24", 352deg, 1966).
mu alpha = +0.455", mu delta = -0.067". SB2 (P = 4.08322d
[00313]). Flares Delta(U) = 0.7 [00344].
FL Aqr BDS 11854 B (A = FK Aqr; B 24", 352deg, 1966).
KV Aqr One deep fading overlapping a brightening trend.
omi Aqr Shell or disk spectrum is observed.
pi Aqr The brightness increased by ~0.2m V
in 1957 - 1975, the star became redder. Balmer
continuum in emission. Rapid changes in emission
lines and in polarization. Existence of a disk
or a shell is possible.
R Aql P var. Max = 2440038 + 297d*E (JD2427850 - 40000).
Since JD2440000 - see Table.
For the whole observed period
Max = 2399190 + 346.932d*n - 0.239303d*n**2;
Pn = 348.980d - 0.554202d*n + 0.000552309d*n**2 [03143].
H2O, OH and SiO maser. Radiobursts.
U Aql B - V: +0.84, +1.24. P var. ADS 12503 A (B 14.00m,
35", 349deg, 1900; one more companion 11.7m V, 2", 230deg,
1934).
W Aql S 6/6e. Composite spectrum near Min light; a companion
(F5 - F8) may exist [03502].
Y Aql Depth of Min II 0.03m. SB1.
RR Aql Maser H2O, OH, SiO.
RT Aql Maser H20, OH, SiO.
SY Aql Maser H2O, OH.
SZ Aql B - V: +1.04, +1.82. P var [02392]. Before JD2420260
P = 17.1359d. Current elements - see Table.
TT Aql B - V: +0.96, +1.62. P var. [02392]. Before JD2418035
P = 13.7518d. Current elements - see Table.
TV Aql P var (changed at ~JD2430000).
Before JD2430000 Max = 2429730 + 237.9d*E.
TW Aql Cycles 65d or 95d are observed during different time
intervals [08714].
UU Aql Mean cycle: 71.3d [04063]; 56d [03144].
UY Aql Cyclic changes of light (P ~400d) with superimposed very
rapid variations are noted in [00504].
VX Aql SC5-/8e. According to [04231], the variable is irregular.
Lithium star.
VZ Aql B - V: +0.61, +1.01.
XZ Aql P var. Min = 2424449.277 + 2.139147d*E
(JD2424380 - 2430300). Since JD2433000 - see Table.
YZ Aql d = 0.03P. P var.
AA Aql Delta(S) = 1.0.
AC Aql P var.
AD Aql CN bands are observed in the spectrum. According to [06928],
the range is 8.83 - 13.42 V.
AE Aql VB A (B 16.6m, 12", 330deg; C 16.9m, 11", 0deg).
The combined light of A, B, C varies in the range
13.9 - 15.8.
AF Aql The period may be two times shorter.
AL Aql d = 0.04P.
AU Aql According to [03146], P = 190d or 380d.
BL Aql P var. Max = 2418538 + 159.65d*E (JD2418529 -
29075). During JD2436420 - 38940 - see Table.
BY Aql P var?
CD Aql Close companion?
CL Aql Sometimes maxima predicted according to the
elements do not occur.
CM Aql Symbiotic spectrum similar to that of Z And [03149].
CR Aql Considerable Blazhko effect is possible.
CS Aql Close companion?
CT Aql According to [06004], only slow irregular variations with
Delta(m) ~0.6 were observed in 1963 - 1968.
CU Aql P var? (Possible change ~JD2423000). Earlier Max = 2418591
+ 203.7d*E.
CV Aql P var?
CW Aql Close companion?
DD Aql Close companion?
DT Aql P var (Change ~JD2425000). Earlier Max = 2423964 + 290.5d*E.
DY Aql P var [06107].
EV Aql P var. Before JD2423900 P = 38.67d. [A/H] = -0.3.
EX Aql P = 117d is also observed.
EZ Aql P var [06107].
FF Aql ADS 11884 A (B 10.37m, 7", 141deg). SB1 (P = 1435d).
FG Aql At the edge of the dark nebula Barnard 130. May be a
physical pair with FH Aql (rho ~20"). According to
[00504], the mean cycle of light variations is 3.5d.
The level of mean light varies.
FH Aql At the edge of the dark nebula Barnard 130. May be a
physical pair with FG Aql (rho ~ 20"). According to
[00504], the mean cycle of light variations is 3.44d.
FK Aql Depth of Min II 0.03m. P var.
FM Aql B - V: +1.12, +1.50.
FN Aql B - V: +1.10, +1.39. P var.
FZ Aql VB A (B 11.5m, 14", 162deg).
GM Aql UV type is possible [00504].
GU Aql d = 0.02P.
GV Aql Nova-like star according to [02089].
GY Aql Maser OH, SiO.
HK Aql Type ISB is not excluded.
HL Aql P var? The 15m star shown in the charts [02274, 06996] with
co-ordinates coincident with those given at the discovery
is constant according to [02274].
IM Aql P var. Before JD2432772 Max = 2428064.707 + 0.4569602d*E.
IO Aql VB A (B = IP Aql, 30", 101deg).
IP Aql VB B (A = IO Aql).
IS Aql Close companion.
KL Aql B - V: +0.78, +1.19, [A/H] = 0.6.
KO Aql d = 0.018P. Min II 8.40. P var. Min = 2427550.565 +
2.863859d*E (JD2426250 - 33000) [02462]; Min =
2433888.366 + 2.863954d*E (JD2433000 - 39000).
current elements - see Table.
KP Aql Min II 10.43; Min II - Min I = 0.50P; DII = DI.
KV Aql During JD2429130 - 31370 - see Table.
During JD2428308 - 28433 the star was faint. Max 2436015
also is not satisfied by the elements.
LU Aql In [03158] P = 102d is given, and the existence of the
variation of mean magnitude with P ~1080d and
Delta(m) = 0.4m was suspected.
MV Aql Close component, the range is given for combined light.
NN Aql Cyclic P variations?
NV Aql Variations of mean light with P ~ 900d - 1000d and
Delta(m) ~0.6m.
OO Aql Min II 9.8. P var. Min I = 2426892.0582 +
0.5067954d*E (1932 - 1934), Min I = 2433925.3762 +
0.5067943d*E [08072]. Since JD2438000 - see Table.
The shape of the light curve varies.
OX Aql Var 2 in the chart for OW Aql.
PP Aql [A/H] = -0.0. CWA type
is not excluded. According to [03161]
P var. Max = 2415229.15 + 24.0147d*E (JD2415228 -
21064), Max = 2426576.14 + 24.074d*E (JD2426576 -
29489). After JD2432040 Max = 2433141.78 + 23.994d*E.
Current elements Max = 2436836.04 + 23.973d*E.
PZ Aql P var? According to [05387], before JD2428075 P = 8.7555d;
P = 8.7504d (JD2428075 - 34725); since JD2434725
P = 8.7573d. See also [02274]. Elements in the Table are
satisfactory after JD2433150. The shape of the light curve
apparently varies.
QS Aql Min II 5.97. VB (A 6.5m; B 6.7m, 0.18", 137deg). P var.
QV Aql The epoch of main Max is given.
QY Aql d = 0.016P. P var?
V0336 Aql B - V: +1.17, +1.55.
V0337 Aql Min II 9.09. P var.
The shape of the light curve varies.
V0340 Aql d = 0.05P. P var.
V0341 Aql P var. Delta(S) = 4.
V0342 Aql ADS 12259 B (A 7.5m; B 20", 14deg); d = 0.032P. P
increases (see also [02265, 04493]). Before JD2435600 Min =
2428023.550 + 3.390842d*E.
Halpha emission observed at Max light [08074]. The shape
of the light curve and d apparently vary. Delta(m)
probably decreases [08075].
V0343 Aql Min II 10.7.
V0346 Aql Min II 9.1. ADS 13438 A (B 11.3m, 2", 245deg).
Elements in the Table are valid af