AAVSO NEWS FLASH No. 17


              THE AMERICAN ASSOCIATION OF VARIABLE STAR OBSERVERS
                   25 Birch Street, Cambridge, MA 02138 USA
                   Tel. 617-354-0484       Fax 617-354-0665
                          INTERNET: aavso@aavso.org

                        * * *  AAVSO NEWS FLASH  * * *

Subject: AK Cnc, AT Cnc, SY Cnc, R CrB             No. 17
         SS Cyg, AM Her, VW Hyi, ER UMa
                                                   May 6, 1996
________________________________________________________________________________

AK CANCRI

The dwarf nova type cataclysmic variable AK Cnc is in outburst as indicated 
by the following observations:

                                       AAVSO Observer
    UT             JD        Mag.        Initials

MAY 2.2021    2450205.7021  <13.6          BTH   
MAY 4.2014    2450207.7014   13.6          BTH   
MAY 5.1917    2450208.6917   13.4          BTH   
MAY 6.2042    2450209.7042   13.6          BTH   
-----------------------------------------------------------------------------

AT CANCRI

The dwarf nova type cataclysmic variable AT Cnc is in outburst as 
indicated by the following observations:

                                       AAVSO Observer
    UT             JD        Mag.        Initials

MAY 1.1979    2450204.6979  <14.0          BTH       
MAY 2.2382    2450205.7382   13.8:         BTH       
MAY 4.1931    2450207.6931   13.2          BTH       
MAY 5.1868    2450208.6868   12.8          BTH       
MAY 6.1986    2450209.6986   13.2          BTH       
-----------------------------------------------------------------------------

SY CANCRI

The dwarf nova type cataclysmic variable SY Cnc is in outburst as 
indicated by the following observations:

                                       AAVSO Observer
    UT             JD        Mag.        Initials

APR 25.0729   2450198.5729   13.6          BRJ       
APR 28.0806   2450201.5806   13.1          BRJ       
APR 29.1986   2450202.6986   12.4:         BTH       
APR 30.1986   2450203.6986   12.6:         BTH       
MAY 1.2125    2450204.7125   12.2          HSG       
MAY 1.2146    2450204.7146   12.1          BTH       
MAY 2.0889    2450205.5889   12.5          MKJ       
MAY 2.2458    2450205.7458   12.0          BTH       
MAY 4.2028    2450207.7028   11.4          BTH       
MAY 5.1931    2450208.6931   11.5          BTH       
MAY 6.1667    2450209.6667   11.2          HSG       
MAY 6.2056    2450209.7056   11.5          BTH       
-----------------------------------------------------------------------------

R CORONAE BOREALIS

R CrB continues to brighten (see AAVSO News Flash No.16) as indicated 
by the following observations:

                                       AAVSO Observer
    UT             JD        Mag.        Initials

APR 30.9326   2450204.4326   11.0          BMM      
MAY 1.1528    2450204.6528   10.9          DIL      
MAY 1.2472    2450204.7472   11.3          HSG      
MAY 2.0521    2450205.5521   10.7          RRB      
MAY 2.3229    2450205.8229   11.0          GMB      
MAY 2.9       2450206.4      10.5          KIL      
MAY 4.867     2450208.367    10.4          DPA
MAY 4.973     2450208.473    10.4          PYG      
MAY 5.873     2450209.373    10.4          DPA
MAY 5.9       2450209.4      10.8          VET      
MAY 5.974     2450209.474    10.5          PYG      
MAY 6.1431    2450209.6431   11.0          HSG      
MAY 6.2264    2450209.7264   10.3          RR       
-----------------------------------------------------------------------------

SS CYGNI

SS Cyg is fading slowly from its recent maximum (see AAVSO News Flash 
No. 16) as indicated by the following observations:

                                       AAVSO Observer
    UT             JD        Mag.        Initials

APR 30.939    2450204.439     8.6          JLT      
MAY 2.2889    2450205.7889    8.6          KMA      
MAY 2.3535    2450205.8535    8.4          GMB      
MAY 2.4771    2450205.9771    8.4          COL      
MAY 2.96      2450206.46      8.3          GUN      
MAY 3.0       2450206.5       8.5          KIL      
MAY 3.2931    2450206.7931    8.6          KMA      
MAY 3.4743    2450206.9743    8.4          COL      
MAY 5.051     2450208.551     8.7          PYG      
MAY 6.050     2450209.55      8.8          PYG      
-----------------------------------------------------------------------------

AM HERCULIS

The magnetic cataclysmic variable AM Her is fluctuating in brightness 
as indicated by the following observations:

                                       AAVSO Observer
    UT             JD        Mag.        Initials

APR 27.059    2450200.559    13.6          SKP      
APR 28.1007   2450201.6007   14.0          BRJ      
APR 28.3139   2450201.8139   13.7          HAV      
APR 28.3264   2450201.8264   13.7          HSG      
APR 29.071    2450202.571    14.0          JLT      
MAY 2.3014    2450205.8014   13.7          KMA      
MAY 3.3139    2450206.8139   13.7          KMA      
MAY 4.983     2450208.483    13.9          PYG      
MAY 5.9       2450209.4      14.4          VET      
MAY 5.985     2450209.485    13.9          PYG      
MAY 6.2069    2450209.7069   13.8          HSG      

This star oscillates between magnitude 12.5 and 14.1 in its "up" state.  
The above observations fall within the fainter end of this range.  Please 
keep an eye on AM Her to see if the "up" state will continue. 
-----------------------------------------------------------------------------

VW HYDRI

The dwarf nova (SU UMa subclass) type cataclysmic variable VW Hyi is 
having a superoutburst (See AAVSO News Flash No. 15 and 16) as indicated by 
observations from Jan Hers, Danie Overbeek and Jan Smit (South Africa) and 
William Liller (Chile).  Excellent sets of CCD(V) data on superhumps have 
been obtained by W. Liller on several nights.

The XTE satellite has been observing VW Hyi since May 2nd and EUVE is 
scheduled to observe it starting May 7.  Both satellites will be observing 
it until May 15.  Observers in the Southern Hemisphere are strongly 
encouraged to keep a close eye on this star and phone in/Fax/e-mail your 
observations to AAVSO so that we can inform the Principal Investigator at 
Lawrence Livermore National Laboratory, California of its behavior.

-----------------------------------------------------------------------------

ER URSAE MAJORIS

The dwarf nova (SU UMa subclass) type cataclysmic variable ER UMa is in 
outburst as indicated by the following observations:

                                       AAVSO Observer
    UT             JD        Mag.        Initials

MAY 4.2250    2450207.725   <14.0          BTH      
MAY 4.952     2450208.452    14.6          PYG      
MAY 5.2118    2450208.7118  <14.0          BTH      
MAY 5.955     2450209.455    13.3          PYG      
MAY 6.2188    2450209.7188   13.3          BTH      
-----------------------------------------------------------------------------

We thank the following contributors for the data that they have provided 
for this News Flash:

BMM - M. Biesmans, Belgium             KIL - L. Kiss, Hungary              
BRJ - J. Bortle, USA                   KMA - M. A. Kamorous, Canada        
BTH - T. Burrows, USA                  LIW - W. Liller, Chile              
COL - P. Collins, USA                  MKJ - J. McKenna, USA               
DIL - W. Dillon, USA                   OB  - D. Overbeek, South Africa     
DPA - A. Diepvens, Belgium             PYG - G. Poyner, England            
GMB - M. Gable, USA                    RR  - R. Royer, USA                 
GUN - J. Gunther, France               RRB - R. Raphael, USA               
HAV - R. Harvan, USA                   SJX - J. Smit, South Africa         
HJN - J. Hers, South Africa            SKP - P. Skalak, Czech Republic     
HSG - G. Hanson, USA                   VET - M. Verdenet, France           
JLT - L. T. Jensen, Denmark      


Please monitor these stars closely and phone-in, fax, or e-mail your 
observations to the AAVSO.

Good observing!
Janet A. Mattei

________________________________________________________________________________

Symbols may include:  < = fainter than magnitude given (variable not seen)
                      : = uncertain
                   CCDV = Charge-coupled device with (V) filter


If you would like to contribute to AAVSO NEWS FLASH, please send
observations of unusual variable star activity to:

                     observations@aavso.org

Those who wish to subscribe (free of charge) or unsubscribe to NEWS FLASH 
may do so by sending a message to:

                     observations@aavso.org

If you would like data from the AAVSO International Database for
research purposes, please send your request to:

        Janet Mattei, AAVSO Director, at aavso@aavso.org

We look forward to including your observations in future editions
of AAVSO NEWS FLASH!

________________________________________________________________________________


Return to HomePage


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