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J/PAZh/26/705    UBV observations of  post-AGB supergiants  (Arkhipova+, 2000)

UBV observations of post-AGB supergiants and peculiarities of their photometric variability. Arkhipova V.P., Ikonnikova N.P., Noskova R.I., Sokol G.V. <Pis'ma Astron. Zh. 26, 705 (2000)> =2000PAZh...26..705A =2000AstL...26..609A
ADC_Keywords: Stars, peculiar ; Stars, supergiant ; Photometry, UBV Abstract: Systematic UBV observations of six variable post-AGB supergiants in 1991-1999 are presented. Objects: ---------------------------------------------------------------------------- RA (2000) DE Designation (File) ---------------------------------------------------------------------------- 18 11 30.7 +27 05 16 V887 Her = GLMP 735=IRAS 18095+2704 (table1.dat) 19 41 08.3 +02 02 31 IRAS 19386+0155 (table2.dat) 20 02 27.3 +30 04 25 V1027 Cyg = HD 333385 (table3.dat) 22 29 10.3 +54 51 06 V354 Lac = HD 235858 (table4.dat) 19 52 52.7 -17 01 50 SAO 163075 = HD 187885 (table5.dat) 20 58 55.7 +49 31 12 IRAS 20572+4919 = EM*VES 351 (table6.dat) ---------------------------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 26 103 UBV-observations V887 Her in 1993-1999 table2.dat 26 76 UBV-observations IRAS19386+0155 in 1993-1999 table3.dat 26 65 UBV-observations V1027 Cyg in 1997-1999 table4.dat 26 72 UBV-observations V354 Lac in 1993-1999 table5.dat 26 77 UBV-observations SAO163075 in 1993-1999 table6.dat 26 70 UBV-observations IRAS20572+4919 in 1994-1999
See also: J/PAZh/27/187 : Light variations in HD 179821 (Arkhipova+, 2001) Byte-by-byte Description of file: table*.dat
Bytes Format Units Label Explanations
1- 7 I7 d JD Julian date 10- 14 F5.2 mag Vmag V magnitude 17- 20 F4.2 mag B-V B-V color index 23- 26 F4.2 mag U-B U-B color index

(End) N. Ikonnikova [GAISH], Veta Avedisova [INASAN] 20-Jun-2001
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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