Tabelle mit allen Bernhard-Variablen im Detail
Quelle: VSNET, Bernhard priv.
Stand: 28.12.2000
Die Benennung der von Klaus Bernhard entdeckten Veränderlichen ist
jetzt offiziell geändert worden, da es eine Namensüberschneidung
gegeben hat. Die korrekte Bezeichnung findet sich in den Überschriften
dieser Tabelle wieder (Brh V**). Aktuelle Informationen zu den Brh-Sternen
finden Sie ab sofort auf der Homepage von Klaus Bernhard
http://mitglied.tripod.de/KlausBernhard/index.html
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## Brh V1
GSC1062.33 195340.19 +092351.6 (2000.0) 10.24 1
GSC1062.33 195340.28 +092350.3 (2000.0) 10.60 1
USNO0975.17237483 195340.187 +092350.20 (2000.0) 10.7 12.1
USNO0975.17237552 195340.239 +092351.01 (2000.0) 10.4 99.9
195340.1 +092351 (2000.0) BeV1 10.5 11.0C EA 1.6160
195340.2 +092351 (2000.0) 1084 0.60 TYC1062.33.1 plx=-30.1(48.2) (0.09 0.12)
## Brh V2
USNO0975.18504733 201144.587 +085516.09 (2000.0) 13.4 16.1
201144.5 +085516 (2000.0) BeV2 12.6 13.6C EA 2.0362?
## Brh V3
GSC5582.545 145117.05 -110943.4 (2000.0) 12.05 0
GSC5582.545 145117.06 -110943.0 (2000.0) 11.60 0
USNO0750.08692370 145117.056 -110943.43 (2000.0) 11.7 12.6
## Brh V4
GSC128.1121 055227.85 +062053.0 (2000.0) 11.86 1
USNO0900.02042842 055227.863 +062052.80 (2000.0) 11.5 14.2
IRAS05497+0620 054947.1 +062014 (1950.0)
F12=0.36 F25=0.25L F60=0.44L F100=3.98L
VAR=-1 LRS=-1
055227.8 +062052 (2000.0) BeV4 11.7 12.2C L:
055227.6 +062049 (2000.0) FSC05497+0620 0.349 0.188 0.609L 6.944L
055228.1 +062054 (2000.0) GCSS170 - 13.0 - -
055228.2 +062052 (2000.0) IRAS05497+0620 0.369 0.250L 0.437L 3.889L -1%
055228.2 +062052 (2000.0) SSC05497+0620 0.369 0.250L 0.437L 3.889L
## Brh V5
GSC144.1300 062040.00 +061608.1 (2000.0) 12.12 1
USNO0900.02778144 062040.034 +061608.03 (2000.0) 11.5 14.0
IRAS06179+0617 061758.9 +061732 (1950.0)
F12=1.20 F25=0.76 F60=0.40L F100=1.44L
VAR=15 LRS=-1
possibly IIIa: variable star with more evolved O-rich c.s. shell
or VIb: variable star with relatively hot dust close to
the star and relatively cold dust at large distance
may be O-rich
or VII: variable star with more evolved C-rich circumstellar shell
062039.9 +061608 (2000.0) BeV5 11.6 12.1C SR:
062039.9 +061607 (2000.0) IRAS06179+0617 1.255 0.758 0.400L 1.427L 15%
062039.9 +061607 (2000.0) SSC06179+0617 1.255 0.758 0.400L 1.427L
062036.0 +061500 (2000.0) (M6III)(Buscombe) - - -
## Brh V6
GSC1008.332 180457.43 +085737.8 (2000.0) 12.19 1
GSC1008.332 180457.43 +085737.5 (2000.0) 12.42 1
USNO0975.10534748 180457.455 +085737.53 (2000.0) 11.5 14.3
180457.3 +085737 (2000.0) BeV6 11.7 12.0C SR: 41 -
180457.1 +085737 (2000.0) FSC18025+0857 0.309 0.120 0.313L 1.655L
180452.8 +085727 (2000.0) IRAS18024+0857 0.429 0.250L 0.400L 1.633L -1%
180452.8 +085727 (2000.0) SSC18024+0857 0.429 0.250L 0.400L 1.633L
## Brh V7
GSC1009.766 180957.39 +085025.0 (2000.0) 10.98 1 N
USNO0975.10779877 180957.392 +085025.00 (2000.0) 11.0 99.9
180957.3 +085024 (2000.0) BeV7 11.6 12.1C EA 2.16252
## Brh V8
GSC1057.1309 194625.07 +084512.3 (2000.0) 11.63 1
USNO0975.16659519 194625.009 +084511.91 (2000.0) 11.8 12.9 *
194625.0 +084512 (2000.0) BeV8 11.7 12.2C S
## Brh V9
GSC171.2059 071152.58 +040405.1 (2000.0) 11.39 6
USNO0900.04485140 071152.588 +040404.64 (2000.0) 12.0 12.0
071152.5 +040405 (2000.0) BeV9 11.4 11.9C EA? - -
## Brh V10
GSC1024.2911 183206.86 +080712.4 (2000.0) 13.28 1
USNO0975.12192664 183206.852 +080712.66 (2000.0) 11.7 15.1
IRAS18297+0804 182943.2 +080456 (1950.0)
F12=0.44 F25=0.25L F60=0.40L F100=2.29L
VAR=-1 LRS=-1
183206.8 +080712 (2000.0) BeV10 12.1 12.5C SR: - -
183207.4 +080710 (2000.0) IRAS18297+0804 0.430 0.250L 0.400L 2.267L -1%
183207.4 +080710 (2000.0) SSC18297+0804 0.430 0.250L 0.400L 2.267L
## Brh V11
USNO0975.12403393 183506.134 +081427.09 (2000.0) 11.6 15.1
183506.0 +081427 (2000.0) BeV11 12.2 12.4C SR: - -
## Brh V12
GSC1010.732 181946.72 +080024.3 (2000.0) 10.88 1
GSC1010.732 181946.86 +080023.5 (2000.0) 11.59 1
USNO0975.11359244 181946.807 +080024.85 (2000.0) 99.9 12.2
181946.7 +080023 (2000.0) BeV12 11.5 11.8C - - -
## Brh V13
GSC140.1831 061856.14 +040919.8 (2000.0) 12.06 6
USNO0900.02715092 061856.167 +040919.40 (2000.0) 12.0 12.6
061856.1 +040919 (2000.0) BeV13 12.1 12.8C EA 1.14962
## Brh V14
GSC959.1397 162449.68 +080414.1 (2000.0) 12.90 1
USNO0975.08430373 162449.698 +080414.44 (2000.0) 12.5 12.9
162449.6 +080414 (2000.0) BeV14 12.6 13.6C RR 0.64465
## Brh V15
GSC396.1710 165129.86 +062226.7 (2000.0) 13.07 1
USNO0900.09085953 165129.912 +062227.03 (2000.0) 12.7 13.3
165129.8 +062226 (2000.0) BeV15 12.7 13.4C RR 0.77892
## Brh V16
USNO0900.11731464 180729.218 +062236.23 (2000.0) 12.0 15.7
IRAS18050+0622 180503.2 +062209 (1950.0)
F12=0.40 F25=0.25L F60=0.40L F100=5.75L
VAR=-1 LRS=-1
180729.1 +062235 (2000.0) BeV16 12.8 13.1C SR - -
180727.9 +062236 (2000.0) FSC18050+0622 0.361 0.176L 0.363L 2.188L
180729.4 +062236 (2000.0) IRAS18050+0622 0.404 0.250L 0.400L 5.911L -1%
180729.4 +062236 (2000.0) SSC18050+0622 0.404 0.250L 0.400L 5.911L
## Brh V17
GSC477.3880 192436.42 +063127.7 (2000.0) 12.67 1
USNO0900.15050706 192436.438 +063128.17 (2000.0) 12.0 13.7
192436.3 +063126 (2000.0) BeV17 12.3 12.7C S: - -
IRAS19221+0626 192210.4 +062613 (1950.0)
F12=0.33 F25=0.30L F60=0.63L F100=8.31L
VAR=-1 LRS=-1
192436.9 +063209 (2000.0) IRAS19221+0626 0.318 0.296L 0.634L 8.460L -1%
192436.9 +063209 (2000.0) SSC19221+0626 0.318 0.296L 0.634L 8.460L
## Brh V18
GSC490.4680 193711.76 +062810.6 (2000.0) 13.08 1
USNO0900.15998453 193711.798 +062810.20 (2000.0) 12.7 13.7
193711.6 +062809 (2000.0) BeV18 12.8 13.1C S: - -
## Brh V19
USNO0975.16432142 194340.262 +103907.21 (2000.0) 12.7 15.4
194340.2 +103906 (2000.0) BeV19 12.4 12.7C SR - -
## Brh V20
GSC1060.2412 193930.58 +104313.8 (2000.0) 13.20 1 N
USNO0975.16097552 193930.598 +104314.00 (2000.0) 12.8 14.8
193930.4 +104312 (2000.0) BeV20 12.7 13.0C SR - -
## Brh V21
GSC1062.2668 195412.75 +103928.5 (2000.0) 13.52 1 N
USNO0975.17284757 195412.723 +103928.21 (2000.0) 12.5 15.7
195412.6 +103927 (2000.0) BeV21 12.2 12.5C SR - -
IRAS19517+1031 195146.8 +103124 (1950.0)
F12=0.58 F25=0.28L F60=0.40L F100=5.75L
VAR=-1 LRS=-1
possibly I: oxygen-rich non-variable star without circumstellar shell
or II: variable star with 'young' O-rich circumstellar shell
or VII: variable star with more evolved C-rich circumstellar shell
or VIa: non-variable star with relatively cold dust at large
distance, may be carbon-rich
195409.4 +103918 (2000.0) IRAS19517+1031 0.575 0.276L 0.400L 5.994L -1%
195409.4 +103918 (2000.0) SSC19517+1031 0.575 0.276L 0.400L 5.994L
## Brh V22
GSC1062.1819 194915.16 +103542.5 (2000.0) 13.13 1
USNO0975.16882756 194915.145 +103542.40 (2000.0) 12.5 15.8
194915.1 +103542 (2000.0) BeV22 12.1 12.4C SR - -
## Brh V23
GSC1076.1805 200936.18 +103909.2 (2000.0) 13.99 1
USNO0975.18380409 200936.204 +103909.23 (2000.0) 12.9 15.8
200936.0 +103908 (2000.0) BeV23 12.6 13.0C SR - -
## Brh V24
GSC1078.852 201813.66 +103754.5 (2000.0) 12.41 1
GSC1078.852 201813.76 +103754.8 (2000.0) 12.18 1
USNO0975.18850999 201813.690 +103754.46 (2000.0) 11.4 14.9
201813.6 +103753 (2000.0) BeV24 11.6 11.9C SR - -
201814.6 +103804 (2000.0) FSC20158+1028 0.224 0.091L 0.347L 1.757L
## Brh V25
GSC1108.961 211021.12 +103600.5 (2000.0) 11.59 1
USNO0975.20406767 211021.142 +103600.44 (2000.0) 12.1 16.0
IRAS21079+1023 210755.5 +102343 (1950.0)
F12=4.36 F25=3.02 F60=0.44 F100=1.00L
VAR=99 LRS=-1
IIIa: variable star with more evolved O-rich c.s. shell
211021.0 +103600 (2000.0) BeV25 12.3 12.8C SR - -
211020.2 +103556 (2000.0) FSC21079+1023 5.130 3.017 0.421 1.359L
211020.7 +103559 (2000.0) IRAS21079+1023 4.170 2.910 0.445 1.000L 99%
211020.7 +103559 (2000.0) SSC21079+1023 4.170 2.910 0.445 1.000L
## Brh V26
GSC1108.2511 210422.38 +102828.4 (2000.0) 13.52 1
USNO0975.20294270 210422.374 +102828.64 (2000.0) 11.4 14.5
210422.2 +102827 (2000.0) BeV26 12.1 12.6C SR - -
210423.4 +102841 (2000.0) FSC21019+1016 0.152 0.131L 0.123L 0.741L
## Brh V27
GSC1076.1332 200300.63 +103455.9 (2000.0) 12.10 1
USNO0975.17946573 200300.592 +103455.31 (2000.0) 11.4 12.0
200300.6 +103455 (2000.0) BeV27 11.5 11.9C E: 0.870? -
## Brh V28
GSC1123.1704 212830.23 +104522.3 (2000.0) 13.16 1
USNO0975.20684593 212830.266 +104522.45 (2000.0) 12.3 12.6
212830.1 +104521 (2000.0) BeV28 12.7 13.2C E 1.28: -
## Brh V29
GSC1139.11 220140.74 +103718.3 (2000.0) 12.71 1
USNO0975.21058934 220140.740 +103718.34 (2000.0) 12.7 13.3
## Brh V30
GSC1172.1452 233232.61 +103320.3 (2000.0) 12.36 1
USNO0975.21637769 233232.645 +103320.99 (2000.0) 12.4 13.2
## Brh V31
BeV31: GSC 718 685
new BeV31 054407.8 N100542 (2000) 11.9 12.1 (CCD) SR
The change in brightness and the red colour
(USNO A2.0: r:11.6 mag, b: 14.1 mag) suggest a SR-variable.
## Brh V32
BeV32: GSC 705 921
new BeV32 053449.6 N101611 (2000) 12.1 12.3 (CCD) SR
The change in brightness and the red colour
(USNO A2.0: r:12.3 mag, b: 15.1 mag) suggest a SR-variable.
## Brh V33
BeV33: GSC 703 625
new BeV33 051452.1 N101107 (2000) 11.7 12.1 (CCD) SR
The change in brightness and the red colour
(USNO A2.0: r:11.2 mag, b: 14.1 mag) suggest a SR-variable.
## Brh V34
BeV34: GSC 768 707
new BeV34 072527.4 N101823 (2000) 11.5 11.8 (CCD) SR
The change in brightness and the red colour
(USNO A2.0: r:11.4 mag, b: 13.8 mag) suggest a SR-variable.
## Brh V35
BeV35 051722.0 N101828 (2000) 12.5 12.9 (CCD)
comments:
BeV35: GSC 703 1930
Comparison star was for all measurements GSC 703 2180 (12.2 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK.
His comment:
GSC 703.1930 has a very strong series of frequencies at n.417
cycles/day.
Marginally the best is 0.41376 days (f=2.417), but the variation is very
sinusoidal and for most the error is very small, about 0.01 mag. It may
be a c-type RR Lyrae variable or perhaps an ellipsoidal variable.
object YYMMDD(UT) mag (ccd) code
BeV35 000111.8944 12.54 BRH.BAV
BeV35 000124.8715 12.88 BRH.BAV
BeV35 000125.9007 12.45 BRH.BAV
BeV35 000126.8979 12.82 BRH.BAV
BeV35 000127.8694 12.65 BRH.BAV
BeV35 000204.8382 12.45 BRH.BAV
BeV35 000210.9090 12.73 BRH.BAV
## Brh V36
BeV36 062454.0 N101405 (J2000) 11.7 12.1(CCD)
comments:
BeV36: GSC 736 1615
Comparison star was for all measurements GSC 736 765 (11.9 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
GSC 736.1615 shows a single series of frequencies around 2.800
cycles/day and its one-day aliases.
This star is probably a weakly eclipsing variable
and the best period is probably 1.256 or 0.555 days (or twice these).
object YYMMDD(UT) mag (CCD) code
BeV36 000111.9403 11.73 BRH.BAV
BeV36 000124.9174 12.10 BRH.BAV
BeV36 000125.9472 11.82 BRH.BAV
BeV36 000126.9444 11.72 BRH.BAV
BeV36 000127.9160 11.78 BRH.BAV
BeV36 000201.9076 11.74 BRH.BAV
BeV36 000203.9375 12.11 BRH.BAV
BeV36 000204.8840 11.72 BRH.BAV
BeV36 000210.9222 11.72 BRH.BAV
## Brh V37
BeV37 065810.8 N101358 (J2000) 12.5 12.9(CCD)
comments:
BeV37: GSC 752 2349
Comparison star was for all measurements GSC 752 2661 (12.6 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
GSC 752.2349 shows a single series of frequencies around 2.804
cycles/day and its one-day aliases, the best are 0.35645 and 0.5540
days.
It may be a c-type RR Lyrae variable or perhaps an ellipsoidal variable.
object YYMMDD(UT) mag (CCD) code
BeV37 000111.9583 12.53 BRH.BAV
BeV37 000124.9354 12.81 BRH.BAV
BeV37 000125.9646 12.67 BRH.BAV
BeV37 000126.9618 12.55 BRH.BAV
BeV37 000127.9333 12.62 BRH.BAV
BeV37 000203.9549 12.91 BRH.BAV
BeV37 000210.9396 12.49 BRH.BAV
## Brh V38
New variable star:
new BeV38 060520.1 N100425 (J2000) 11.6 12.1(CCD)
comments:
BeV38: GSC 721 2377
Comparison star was for all measurements GSC 721 2390 (12.0 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
GSC721.2377 looks like an eclipsing binary and four possible periods
emerge at 0.365, 0.636, 1.363 and 1.634 cycles/day.
These are 2.74, 1.57, 0.73 and 0.61 days, but the real period may be
twice any of these, although I would guess it's in the 1 - 2 day
range.
object YYMMDD(UT) mag (CCD) code
BeV38 000111.9271 11.57 BRH.BAV
BeV38 000124.9042 11.57 BRH.BAV
BeV38 000125.9340 11.67 BRH.BAV
BeV38 000126.9313 11.73 BRH.BAV
BeV38 000127.9028 11.59 BRH.BAV
BeV38 000203.9243 12.07 BRH.BAV
BeV38 000207.8764 11.59 BRH.BAV
BeV38 000210.9090 11.58 BRH.BAV
## Brh V39
New variable star:
new BeV39 070100.4 +100346 (J2000) 11.5 11.8(CCD)
comments:
BeV39: GSC 752 542
Comparison star was for all measurements GSC 752 2579 (11.1 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
GSC 752.542 is probably a very short period variable, delta Sct or
similar. The marginally best period is 0.15923 days but the one-day
aliases are almost equally likely.
object YYMMDD(UT) mag (CCD) code
BeV39 000111.9681 11.83 BRH.BAV
BeV39 000124.9451 11.52 BRH.BAV
BeV39 000125.9750 11.76 BRH.BAV
BeV39 000126.9722 11.70 BRH.BAV
BeV39 000127.9438 11.62 BRH.BAV
BeV39 000203.9688 11.53 BRH.BAV
BeV39 000210.9500 11.64 BRH.BAV
## Brh V40
New variable star:
new BeV40 071334.1 +101513 (J2000) 11.1 11.6(CCD)
comments:
BeV40: GSC 766 1248
Comparison star was for all measurements GSC 766 142 (11.8 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
GSC 766.1248 has a very strong series of frequencies with the best
periods 0.77693 and 0.43726 days. I think this one may turn out to be an
RR
Lyrae
variable.
object YYMMDD(UT) mag (CCD) code
BeV40 000111.9736 11.24 BRH.BAV
BeV40 000124.9507 11.13 BRH.BAV
BeV40 000125.9806 11.28 BRH.BAV
BeV40 000126.9778 11.63 BRH.BAV
BeV40 000127.9493 11.33 BRH.BAV
BeV40 000210.9556 11.29 BRH.BAV
## Brh V41
New variable star:
new BeV41 071910.8 +100252 (J2000) 12.5 12.9(CCD) SR
comments:
BeV41: GSC 767 2017
Comparison star was for all measurements GSC 767 1861 (11.8 mag),
which was checked to be constant.
The change in brightness and the red colour
(USNO A2.0: r:12.0 mag, b: 14.9 mag) suggest a SR-variable.
object YYMMDD(UT) mag (CCD) code
BeV41 000111.9819 12.88 BRH.BAV
BeV41 000124.9590 12.84 BRH.BAV
BeV41 000126.9743 12.81 BRH.BAV
BeV41 000127.9458 12.69 BRH.BAV
BeV41 000210.9639 12.48 BRH.BAV
BeV41 000214.9458 12.45 BRH.BAV
BeV41 000227.9174 12.84 BRH.BAV
## Brh V42
New variable star:
new BeV42 072633.2 +100356 (J2000) 12.3 12.6(CCD) SR
comments:
BeV42: GSC 768 618
Comparison star was for all measurements GSC 768 1032 (11.6 mag),
which was checked to be constant. The change in brightness and the
red colour (USNO A2.0: r:12.1 mag, b: 14.9 mag) suggest a SR-variable.
object YYMMDD(UT) mag (CCD) code
BeV42 000124.9549 12.58 BRH.BAV
BeV42 000125.9847 12.59 BRH.BAV
BeV42 000126.9819 12.55 BRH.BAV
BeV42 000127.9535 12.54 BRH.BAV
BeV42 000210.9597 12.55 BRH.BAV
BeV42 000214.9417 12.44 BRH.BAV
BeV42 000227.9139 12.29 BRH.BAV
## Brh V43
New variable star:
new BeV43 051244.8 +101510 (J2000) 11.9 12.4(CCD)
comments:
BeV43: GSC 702 1892
Comparison star was for all measurements GSC 702 1438 (12.4 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
There is a strong series of spikes in the periodogram with 1.3034
and 0.10966 being the strongest. It could be almost any type of variable
at this stage.
object YYMMDD(UT) mag (CCD) code
BeV43 000111.8847 11.98 BRH.BAV
BeV43 000124.8618 11.90 BRH.BAV
BeV43 000125.8910 12.43 BRH.BAV
BeV43 000126.8882 12.23 BRH.BAV
BeV43 000204.8285 11.87 BRH.BAV
BeV43 000210.8660 11.92 BRH.BAV
BeV43 000227.8201 11.90 BRH.BAV
## Brh V44
New variable star:
new BeV44 114545.5 +115208 (J2000) 13.4 14.2(CCD)
comments:
BeV44: GSC 867 545
Comparison star was for all measurements GSC 867 289 (13.0 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
It shows a strong series of period at about equal strength,
however I suspect it may be an RR Lyrae with a period
about 0.68 days.
object YYMMDD(UT) mag (CCD) code
BeV44 000505.9000 14.18 BRH.BAV
BeV44 000506.9062 13.90 BRH.BAV
BeV44 000507.8979 14.16 BRH.BAV
BeV44 000510.8882 13.68 BRH.BAV
BeV44 000513.9173 14.06 BRH.BAV
BeV44 000514.9027 13.38 BRH.BAV
BeV44 000516.9159 13.40 BRH.BAV
