J/A+AS/116/257      Variability in O-stars wind (Kaper+, 1996)

Long- and short-term variability in O-star winds I. Time series of UV spectra for 10 bright O stars. Kaper L., Henrichs H.F., Nichols J.S., Snoek L.C., Volten H., Zwarthoed G.A.A. <Astron. Astrophys. Suppl. Ser. 116, 257 (1996)> =1996A&AS..116..257K 1996A&AS..116..257K (SIMBAD/NED BibCode)
ADC_Keywords: Stars, early-type ; Spectra, ultraviolet Keywords: stars: early-type - stars: mass loss - ultraviolet: stars Description: The tables below list the Log of IUE observations incorporated in the paper. The table number corresponds to the figure number in the paper. The involved O star and the observing period are mentioned in the table header. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table 50 625 IUE observations -------------------------------------------------------------------------------- Byte-by-byte Description of file: table -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- Figno Figure number in the paper 5- 12 A8 "DD/MM/YY" Date Observation date 14- 15 I2 --- Seq Sequence number 17- 21 I5 --- Ident Identification number of the observation obtained with the Short Wavelength Prime camera on IUE 25- 26 I2 h ObsH Start time of the observation (hour) 28- 29 I2 min ObsM Start time of the observation (min) 32- 33 I2 min ExpM Exposure time (min) 35- 36 I2 s ExpS Exposure time (sec) 40- 50 F11.3 d HJD Julian Day at mid-exposure --------------------------------------------------------------------------------
(End) Patricia Bauer [CDS] 04-Jan-1996
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