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J/A+A/258/423 Spectrum of KQ Pup (Muratorio+ 1992)
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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
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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:
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RA (2000) DE Designation(s)
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07 33 48.0 -14 31 26 KQ Pup = HD 60414 (M2III)
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File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 78 491 The spectrum
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See also:
J/A+AS/92/685 : Optical and UV Spectrum of KQ Pup (Altamore+ 1992)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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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
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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.
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(End) Francois Ochsenbein [CDS] 19-Feb-1993