J/A+AS/108/561 P Cygni spectrum in 1985 (Markova, 1994)
How did the spectrum of P Cygni look in 1985? Spectral atlas with complete line
identifications in the wavelength range from 3550 to 4800A
MARKOVA N.
<Astron. Astrophys. Suppl. Ser. 108, 561 (1994)>
=1994A&AS..108..561M 1994A&AS..108..561M (SIMBAD/NED Reference)
ADC_Keywords: Stars, emission; Spectra, ultraviolet
Keywords: stars: P Cygni - line identification - stars: mass loss - atlases
File Summary:
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File Name Lrecl Records Explanations
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ReadMe 80 . This file
table1 69 707 P Cygni spectrum - wavelengths and
identifications
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Byte-by-byte Description of file: table1
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Bytes Format Units Label Explanations
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2- 8 F7.2 0.1nm LamObs Observational wavelengths
10 A1 --- u_LamObs [? ] '?' indicates an uncertain feature
13 A1 --- a/e [ae ] Nature of the line:
a = absorption, e = emission
14 A1 --- n_LamObs [ )] When two or more spectral features are
believed to be formed by the same line or
lines, the different features are connected
by round brackets.
17- 21 F5.2 0.1nm LamLab []? Laboratory wavelengths
25- 36 A12 --- Ion Ion identification
37 A1 --- n_Ion [* ] '*' marks the most important contributor
to a blend
41- 43 A3 --- Rem1 Remarks (1)
47- 48 A2 --- Rem2 Additional remarks (2)
52- 53 A2 --- Overlap "--" marks the area of overlapping of
forbidden and permitted line
55- 69 A15 --- Forbidden Identification of forbidden lines
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Note (1): new = newly identified line
1 = line observed by de Groot (1969)
2 = line observed by Stahl et al. (1993)
Note (2): IS = interstellar line
bl = blend
1 = first absorption component
2 = second absorption component
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References: De Groot, M., 1969, Bull. Astron. Inst. Net., 20, 225
Stahl, O., Mandel, H., Wolf, B., 1993, A&AS, 99, 167
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(End) Patricia Bauer [CDS] 26-Jul-1994