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J/PAZh/23/277       Optical variability of WW Vul         (Zaitseva+, 1997)

On the origin of optical variability of WW Vulpeculae. Zaitseva G.V., Lyutyi V.M. <Pis'ma Astron. Zh. 23, 277 (1997)> =1997PAZh...23..277Z =1997AstL...23..242Z
ADC_Keywords: Stars, variable; Photometry, UBV Abstract: The UBV observations of WW Vul performed between 1983 and 1993 are presented. All UBV observations of WW Vul are reduced to GAISh photometric system. Object: -------------------------------------- RA (2000) DE Designation -------------------------------------- 19 35 59.6 +21 12 33 WW Vul -------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table.dat 30 1074 UBV photometry of WW Vul
Byte-by-byte Description of file: table.dat
Bytes Format Units Label Explanations
1- 11 F11.3 d HJD [2439650/2449296] Julian date 14- 18 F5.2 mag Vmag V magnitude 21- 24 F4.2 mag B-V B-V color index 27- 30 F4.2 mag U-B U-B color index

(End) Veta Avedisova [INASAN] 15-Feb-1999
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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