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 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:
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RA (2000) DE Designation(s)
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11 43 38.3 +71 41 20 DO Dra = V* YY Dra
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table3.dat 21 1511 R observations obtained at the 1m telescope of
the MtLemmon observatory, Korea
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Byte-by-byte Description of file: table3.dat
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Bytes Format Units Label Explanations
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1- 13 F13.5 d HJD Date of observation
15- 21 F7.4 mag Rmag R magnitude
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Acknowledgements:
Ivan Andronov, tt_ari(at)ukr.net
(End) Patricia Vannier [CDS] 27-Jul-2008