[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]

[vsnet-alert 697] CVC 127 (EG Cnc, EY Cyg, V701 Tau, BZ UMa)



BELGIAN ASTRONOMICAL SOCIETY V.V.S. -  Working Group Variable Stars
Cataclysmic Variables Circular No.127              1997, January 27
Ed.: T. Vanmunster, Walhostraat 1A, 3401 Landen, BELGIUM
     Internet: tvanmuns@innet.be                  TEL. 32-11-831504
     CBA Belgium Web Page : http://vsnet.astro.columbia.edu/~cba/be
===================================================================

EG Cnc [UGWZ, 11.9v - 17:v]
===========================

N.Makiguchi, Kanagawa, Japan, Gary Poyner, Birmingham, UK and Lasse 
Jensen, CBA Denmark report yet another rebrightening of EG Cnc. Their 
observations have been included in the photometric summary below.

-------------------------------------------
DATE (UT)       MAGN   MS  OBSERVER
-------------------------------------------

1996 12 06.760   12.9  mv   Watanabe
1996 12 07.630   12.6  mv   Watanabe
1996 12 21.722   13.1  mv   Watanabe
1996 12 21.788   13.1  mv   Watanabe
1997 01 07.024   15.7  mv   Jensen
1997 01 09.142   16.26 CV   Zissell 
1997 01 09.193  <14.1  mv   Hanson
1997 01 09.618  <15.2  mv   Watanabe
1997 01 09.660   15.67 mv   Koshiro
1997 01 10.068   13.17 CU   Jensen
1997 01 10.181   13.8  mv   Hanson
1997 01 10.212   13.7  mv   Hanson
1997 01 10.260   13.8  mv   Hanson
1997 01 10.292   13.5  mv   Shaw
1997 01 10.492   13.8  mv   Takahashi
1997 01 10.538   13.7  mv   Takahashi
1997 01 10.615   13.6  mv   Takahashi
1997 01 10.653   13.4  mv   Itoh
1997 01 10.656   14.03 mv   Koshiro
1997 01 10.748   13.7  mv   Itoh
1997 01 10.760   13.96 CV   Ouda
1997 01 10.84    14.7  mv   Kinnunen
1997 01 10.842   13.8  mv   Itoh
1997 01 11.1538  14.67 CV   Zissell
1997 01 11.1632  14.0  mv   Stewart
1997 01 11.251   14.4: mv   Hanson
1997 01 11.298   14.7: mv   Hanson
1997 01 11.581   14.6: mv   Takahashi
1997 01 11.597  <14.0  mv   Makiguchi
1997 01 11.610  <14.8  mv   Itoh
1997 01 11.635  <14.2  mv   Makiguchi
1997 01 11.694   15.29 CV   Ouda
1997 01 11.946  <14.0  mv   Jensen
1997 01 12.03   <14.9  mv   Pietz
1997 01 12.210  <14.6  mv   Hanson
1997 01 12.596  <14.2  mv   Itoh     
1997 01 12.659   16.27 CV   Ouda
1997 01 13.678   16.21 CV   Ouda
1997 01 13.917  <14.6  mv   Poyner
1997 01 13.946  <13.9  mv   Vanmunster
1997 01 13.98   <14.8  mv   Pietz
1997 01 14.257  <14.6  mv   Shaw
1997 01 14.8722  15.6  mv   Jensen
1997 01 14.98   <15.0  mv   Pietz
1997 01 14.990  <15.1  mv   Poyner
1997 01 15.005  <15.5  mv   Vanmunster
1997 01 15.453  <14.0  mv   Takahashi
1997 01 15.729   16.23 CV   Ouda
1997 01 15.898  <13.9  mv   Vanmunster
1997 01 16.14   <13.7  mv   Schmeer
1997 01 16.148  <15.2  mv   Vanmunster
1997 01 16.284   16.23 CV   Kemp
1997 01 16.559   15.33 CV   Koshiro
1997 01 16.83    13.5  mv   Pietz
1997 01 16.833   13.0: mv   Schmeer
1997 01 16.936   13.6  CU   Vanmunster
1997 01 16.96    13.5  mv   Pietz
1997 01 17.135   13.3  mv   Schmeer
1997 01 17.254   13.6  CU   Vanmunster
1997 01 17.455   13.7  mv   Takahashi
1997 01 17.497   13.6  mv   Takahashi
1997 01 17.585   13.3  mv   Itoh
1997 01 17.773   13.9  mv   Watanabe
1997 01 17.8187  13.50 CU   Jensen
1997 01 17.863   13.8  mv   Itoh
1997 01 17.875   14.3  mv   Poyner
1997 01 17.961   14.2  mv   Poyner
1997 01 18.1277  14.27 CU   Jensen
1997 01 18.508  <14.6  mv   Hanson
1997 01 18.608  <14.0  mv   Makiguchi
1997 01 19.474  <14.6  mv   Hanson
1997 01 19.798   16.30 CV   Ouda
1997 01 20.586  <13.7  mv   Itoh
1997 01 20.669   16.18 CV   Ouda
1997 01 20.88   <15.1  mv   Kinnunen
1997 01 22.608  <13.5  mv   Itoh
1997 01 22.665  <13.4  mv   Watanabe
1997 01 24.7791  16.4  mv   Jensen
1997 01 24.80   <14.1  mv   Kinnunen
1997 01 25.568  <13.5  mv   Itoh
1997 01 25.597  <14.0  mv   Makiguchi
1997 01 25.7347  15.2  mv   Jensen
1997 01 25.854  <14.1  mv   Poyner
1997 01 26.2048  13.85 mv   Jensen
1997 01 26.542   13.5  mv   Makiguchi
1997 01 26.9583  13.7  mv   Poyner



EY Cyg [UGSS, 11.4v - 15.5v]
============================

Following the outburst notification in CVC 125, we herewith present
a first photometric overview :

-------------------------------------------
DATE (UT)       MAGN   MS  OBSERVER
-------------------------------------------
1997 01 10.082  <14.5   mv  Hanson
1997 01 11.298   14.7:  mv  Hanson
1997 01 11.71    12.8:  mv  Pietz
1997 01 11.72    12.8   mv  Pietz
1997 01 11.73    12.8   mv  Pietz
1997 01 11.75    12.8   mv  Pietz
1997 01 11.965   13.1   mv  Dyck
1997 01 12.097   12.7   mv  Hanson
1997 01 12.104   12.7   mv  Hanson
1997 01 12.118   12.7   mv  Hanson
1997 01 12.46    12.0   mv  Dyck
1997 01 12.715   12.5:  mv  Schmeer
1997 01 12.731   12.4   mv  Schmeer
1997 01 13.71    12.1   mv  Pietz
1997 01 13.740   12.0   mv  Poyner
1997 01 13.751   12.1   mv  Broens
1997 01 14.67    12.1   mv  Kinnunen
1997 01 14.7020  11.88  CU  Jensen
1997 01 14.71    11.5   mv  Pietz
1997 01 14.754   11.7   mv  Poyner
1997 01 15.71    11.5   mv  Pietz
1997 01 15.778   12.0   mv  Broens
1997 01 16.67    12.0   mv  Kinnunen
1997 01 16.72    11.5   mv  Pietz
1997 01 17.757   12.1   mv  Poyner
1997 01 18.546   12.1   mv  Hanson 
1997 01 19.093   12.3:  mv  Hanson
1997 01 20.65    12.1   mv  Kinnunen
1997 01 24.081  <12.2   mv  Hanson
1997 01 24.68    12.8   mv  Kinnunen
1997 01 25.749   12.8   mv  Poyner
1997 01 25.079  <12.5   mv  Hanson



V701 Tau [UGSU, 15.0p - <21p]
=============================

The V701 Tau outburst, announced in CVC 124, is a superoutburst,
according to time-series CCD photometry observations at Ouda
Station, Japan and CBA Belgium Observatory.

D. Nogami, Ouda Observatory, Japan reports : "Our 3hr CCD photometry 
on 1997 January 12 at Ouda Station revealed fully developed super-
humps with an amplitude of about 0.2 mag in V701 Tau, proving the 
current outburst to be a superoutburst next to the one observed in 
1995 December/1996 January (see, T. Kato, vsnet-alert 303). This 
suggests that the recurrence time of the superoutburst (supercycle) 
in V701 Tau is about 370 days (or 1/N)."
                                        
Independent CCD photometry at CBA Belgium on January 11/12 and 
January 12/13 confirms these findings. The short duration of the 
observing sessions, combined with poor atmospheric conditions,
prevented the deduction of a secure superhump period. 

-------------------------------------------
DATE (UT)       MAGN   MS  OBSERVER
-------------------------------------------
1997 01 03.044  <14.7   mv  Poyner
1997 01 11.941   15.7   CU  Vanmunster
1997 01 12.0282  15.6   CU  Vanmunster
1997 01 12.505   15.35  CV  Ouda
1997 01 12.782   15.7   CU  Vanmunster
1997 01 12.847   15.7   CU  Vanmunster
1997 01 13.461   15.46  CV  Ouda
1997 01 13.770   15.9   CU  Vanmunster
1997 01 13.861   14.9   mv  Poyner
1997 01 13.965   15.8   CU  Vanmunster
1997 01 14.7444  15.32  CU  Jensen
1997 01 14.951   15.3   mv  Poyner
1997 01 15.469   15.53  CV  Ouda
1997 01 25.817  <15.3   mv  Poyner


BZ UMa [UGSU:, 10.5v - 17.8v]
=============================

Unfiltered time-series CCD photometry at the CBA Belgium Observatory
(using a 25-cm f/6.3 telescope and ST-7 CCD) on January 09/10 and
January 11/12 did not reveal any superhumps. We therefore must
conclude that the present outburst has again been a normal one.
The variable has now returned to minimum light.

-------------------------------------------
DATE (UT)       MAGN   MS  OBSERVER
-------------------------------------------
1997 01 09.194   14.4: mv   Hanson
1997 01 09.196   14.3: mv   Hanson
1997 01 09.202   14.2  mv   Hanson
1997 01 09.206   14.1  mv   Hanson
1997 01 09.211   14.0  mv   Hanson
1997 01 09.214   14.0  mv   Hanson
1997 01 09.217   13.9  mv   Hanson
1997 01 09.221   13.8  mv   Hanson
1997 01 09.224   13.7  mv   Hanson
1997 01 09.229   13.6  mv   Hanson
1997 01 09.232   13.5  mv   Hanson
1997 01 09.235   13.4  mv   Hanson
1997 01 09.241   13.3  mv   Hanson
1997 01 09.244   13.2  mv   Hanson
1997 01 09.247   13.2  mv   Hanson
1997 01 09.250   13.1  mv   Hanson
1997 01 09.253   13.1  mv   Hanson
1997 01 09.256   13.0  mv   Hanson
1997 01 09.262   12.9  mv   Hanson
1997 01 09.266   12.9  mv   Hanson
1997 01 09.272   12.9  mv   Hanson
1997 01 09.277   12.8  mv   Hanson
1997 01 09.531   11.7  mv   Hanson
1997 01 09.560   11.6  mv   Hanson
1997 01 09.749   11.49 CU   Jensen 
1997 01 09.791   11.9  CU   Vanmunster
1997 01 09.820   11.9  CU   Vanmunster
1997 01 09.945   11.5  mv   Jensen
1997 01 10.083   11.4  mv   Hanson
1997 01 10.174   11.5  mv   Hanson
1997 01 10.210   11.9  mv   Hanson
1997 01 10.262   11.7  mv   Hanson
1997 01 10.724   12.59 mv   Koshiro
1997 01 10.7861  12.23 CU   Jensen
1997 01 10.825   12.5  mv   Itoh
1997 01 10.843   12.62 CV   Ouda
1997 01 10.83    12.3  mv   Kinnunen
1997 01 11.1646  13.0  mv   Scovil
1997 01 11.1819  12.3  mv   Stewart
1997 01 11.1854  12.6  mv   Bortle
1997 01 11.246   12.7  mv   Hanson
1997 01 11.283   12.9  mv   Hanson
1997 01 11.631   12.5  mv   Makiguchi
1997 01 11.765   13.9  CU   Vanmunster
1997 01 11.81    13.9  mv   Pietz
1997 01 11.812   13.7  mv   Jensen
1997 01 11.85    14.0  mv   Pietz
1997 01 11.88    13.8  mv   Pietz
1997 01 11.93    13.9  mv   Pietz
1997 01 11.934   14.2  CU   Vanmunster
1997 01 11.97    14.0  mv   Pietz
1997 01 11.984   14.2  mv   Vanmunster
1997 01 12.00    14.3  mv   Pietz
1997 01 12.109   13.8  mv   Hanson
1997 01 12.817   15.07 CV   Ouda
1997 01 13.0465  15.5  mv   Bortle
1997 01 13.809   15.66 CV   Ouda
1997 01 13.846  <13.7  mv   Vanmunster
1997 01 13.868  <15.4  mv   Poyner
1997 01 14.7354  15.75 CU   Jensen
1997 01 14.960  <15.4  mv   Poyner
1997 01 15.821   15.89 CV   Ouda
1997 01 15.834  <14.5  mv   Broens
1997 01 16.147  <13.7  mv   Vanmunster
1997 01 17.904  <13.7  mv   Poyner


Tonny Vanmunster

VSNET Home Page

Return to Daisaku Nogami


vsnet-adm@kusastro.kyoto-u.ac.jp