J/A+AS/93/189   uvby-beta photometry of AE UMa, RV Ari, BP Peg (Rodriguez+ 1992)

Stromgren photometry of three double mode high amplitude Delta Scuti stars RODRIGUEZ E., ROLLAND A., LOPEZ DE COCA P., GARCIA-LOBO E., SEDANO J.L. <Astron. Astrophys. Suppl. Ser. 93, 189 (1992)> =1992A&AS...93..189R 1992A&AS...93..189R
Keywords: stars: variable - stars: delta Scu - photometry File Summary -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2 42 229 Standard uvby (AE UMa - BD+44 1898) table3 21 59 Standard Hbeta(AE UMa) table4 42 140 Standard uvby (RV Ari - HD 14107) table5 21 40 Standard Hbeta(RV Ari) table6 42 299 Standard uvby (BP Peg - HD 205542) table7 21 149 Standard Hbeta(BP Peg) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2 table4 table6 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 14 F12.4 day HJD Heliocentric Julian Day 16- 21 F6.3 mag Du Stroemgren filter magnitude difference 23- 28 F6.3 mag Dv " 30- 35 F6.3 mag Db " 37- 42 F6.3 mag Dy " -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3 table5 table7 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 4- 15 F12.4 day HJD Heliocentric Julian Day 17- 21 F5.3 mag H-beta Standard Hbeta --------------------------------------------------------------------------------
(End) [CDS] 19-Mar-1993
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