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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 (SIMBAD/NED Reference)
ADC_Keywords: Stars, emission; Spectra, ultraviolet Keywords: stars: P Cygni - line identification - stars: mass loss - atlases File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 69 707 P Cygni spectrum - wavelengths and identifications
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
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
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
References: De Groot, M., 1969, Bull. Astron. Inst. Net., 20, 225 Stahl, O., Mandel, H., Wolf, B., 1993, A&AS, 99, 167
(End) Patricia Bauer [CDS] 26-Jul-1994
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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