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J/A+A/258/423          Spectrum of KQ Pup     (Muratorio+ 1992)

The spectrum of the VV Cep star KQ Puppis (Boss 1985). IV. The Fe II spectrum, level population and spectral synthesis Muratorio G., Viotti R., Friedjung M., Baratta G.B., Rossi C. <Astron. Astrophys. 258, 423-431 (1992)> =1992A&A...258..423M
ADC_Keywords: Binaries, spectroscopic; Spectroscopy; Spectra, ultraviolet ; Equivalent widths Keywords: atomic and molecular processes - lines: formation - stars: binaries - spectroscopic: stars - stars: emission line - stars: individual Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 07 33 48.0 -14 31 26 KQ Pup = HD 60414 (M2III) ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 78 491 The spectrum
See also: J/A+AS/92/685 : Optical and UV Spectrum of KQ Pup (Altamore+ 1992) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
7 A1 --- A/E [AE] Nature of the line: A = absorption, E = emission. 10- 16 F7.2 0.1nm Lab Laboratory wavelength (in A) of the transition. 18- 23 F6.3 --- Log.gf Log gf (from Kurucz 1981). 26- 30 I5 cm-1 E.P. Excitation potential of the lower level. 33- 35 F3.1 --- JL J number of the lower level. 37- 39 F3.1 --- JU J number of the upper level. 41- 44 A4 --- MULT Multiplet number according to Moore (1945) and Moore (1950), labeled with "o". "K" denotes a transition listed by Kurucz (1981). 46- 48 I3 10-16W/m2 F1 *? Emission line flux in 10-13 erg.cm-2.s-1 49 A1 --- u_F1 [:Sp] Uncertainty flag (:) on F1, or S for saturated p for a transition contributing to the previous flux 51- 54 I4 0.1pm W1 ? Equivalent width (in mA) in February 1979. 55 A1 --- u_W1 [:Sp] Uncertainty flag on W1 (as in col. 49) 57- 59 I3 10-16W/m2 F2 ? Dereddened emission line flux in February 1980. 60 A1 --- u_F2 [:Sp] Uncertainty flag on F2 (as in col. 49) 62- 65 I4 0.1pm W2 ? Equivalent width in February 1980. 66 A1 --- u_W2 [:Sp] Uncertainty flag on W2 (as in col. 49) 69- 78 A10 --- Rem *Remarks
Note on F1: the flux is corrected corrected for an interstellar extinction of E(B-V)=0.14 measured in the February 1979 IUE spectrum. Note on Rem: Remarks include: bl = more than one transition contribute to the line. (indicated with "...") broad = broad spectral feature. opt = optical transition (Moore 1945). R.M. = IUE reseau mark.

(End) Francois Ochsenbein [CDS] 19-Feb-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

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