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J/A+A/486/855       R light curve of DO Dra                  (Andronov+, 2008)
Multiple timescales in cataclysmic binaries.
The low-field magnetic dwarf nova DO Draconis.
    Andronov I.L., Chinarova L.L., Han W., Kim Y., Yoon J.-N.
   <Astron. Astrophys., 486, 855-865 (2008)>
   =2008A&A...486..855A
ADC_Keywords: Binaries, cataclysmic ; Photometry

Keywords: novae, cataclysmic variables - stars: dwarfs novae -
          stars: binaries: general - stars: variables: general -
          stars: magnetic field - accretion, accretion disks

Abstract:
    We study the variability of the cataclysmic variable DO Dra, on
    time-scales of between minutes and decades.

    The observations were obtained at the Korean 1m telescope at the Mt.
    Lemmon in 2006-2007, 14 observational runs cover 45h. Additionally, we
    have used 1509 patrol observations from the international AFOEV and
    VSOLJ databases.
Objects:
    ---------------------------------------------
       RA   (2000)   DE      Designation(s)
    ---------------------------------------------
    11 43 38.3   +71 41 20   DO Dra = V* YY Dra
    ---------------------------------------------

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
table3.dat        21     1511   R observations obtained at the 1m telescope of
                              the MtLemmon observatory, Korea


Byte-by-byte Description of file: table3.dat

   Bytes Format Units   Label     Explanations

   1- 13  F13.5 d       HJD       Date of observation
  15- 21  F7.4  mag     Rmag      R magnitude


Acknowledgements:
    Ivan Andronov, tt_ari(at)ukr.net
(End)                                      Patricia Vannier [CDS]    27-Jul-2008