J/A+AS/104/509 Stark broadening of Lyman and Balmer lines (Stehle 1994)
Stark broadening of hydrogen Lyman and Balmer lines in the conditions of
stellar envelopes
STEHLE C.
<Astron. Astrophys. Suppl. Ser. 104, 509 (1994)>
=1994A&AS..104..509S 1994A&AS..104..509S
Keywords: atomic data - atomic processes - line: profiles
Historical Notes:
04-Jan-1994: First preparation
10-May-1994: Correction in tabl1-3 (call from Chantal Stelhe)
Last row with Ne=1.000E+15, T=1.000E+04:
values of Dalpha, IDH+ and ISH+ were erroneous.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
tabl1-1 126 394 Lyman alpha (1-2) H+, He+ and Ar+ perturbers
(lambda = 1215.68, Kalpha = 6.731E-06)
tabl1-2 126 381 Lyman beta (1-3) H+, He+ and Ar+ perturbers
(lambda = 1025.73, Kalpha = 3.587E-05)
tabl1-3 126 365 Lyman gamma (1-4) H+, He+ and Ar+ perturbers
(lambda = 972.55, Kalpha = 7.965E-05)
tabl1-4 126 366 Lyman delta (1-5) H+, He+ and Ar+ perturbers
(lambda = 949.75, Kalpha = 1.563E-04)
tabl1-5 126 391 Lyman epsilon (1-6) H+, He+ and Ar+ perturbers
(lambda = 937.81, Kalpha = 2.651E-04)
tabl1-6 126 367 Lyman (1-7) H+, He+ and Ar+ perturbers
(lambda = 930.76, Kalpha = 4.212E-04)
tabl1-7 126 364 Lyman (1-8) H+, He+ and Ar+ perturbers
(lambda = 926.24, Kalpha = 6.238E-04)
tabl1-8 74 286 Lyman (1-9) H+ perturbers
(lambda = 923.16, Kalpha = 8.885E-04)
tabl1-9 77 208 Lyman (1-10) H+ perturbers
(lambda = 65 Kalpha = 6.731E-06)
tabl1-10 77 208 Lyman (1-11) H+ perturbers
(lambda = 919.36, Kalpha = 1.616E-03)
tabl1-11 77 130 Lyman (1-12) H+ perturbers
(lambda = 918.14, Kalpha = 2.093E-03)
tabl1-12 77 130 Lyman (1-13) H+ perturbers
(lambda = 917.19, Kalpha = 2.662E-03)
tabl1-13 75 52 Lyman (1-14) H+ perturbers
(lambda = 916.44, Kalpha = 3.319E-03)
tabl2-1 126 360 Balmer alpha (2-3) H+, He+ and Ar+ perturbers
(lambda = 6564.70, Kalpha = 2.564E-03)
tabl2-2 126 406 Balmer beta (2-4) H+, He+ and Ar+ perturbers
(lambda = 4862.74, Kalpha = 7.062E-03)
tabl2-3 126 402 Balmer gamma (2-5) H+, He+ and Ar+ perturbers
(lambda = 4341.73, Kalpha = 1.189E-02)
tabl2-4 126 358 Balmer delta (2-6) H+, He+ and Ar+ perturbers
(lambda = 4102.94, Kalpha = 1.944E-02)
tabl2-5 126 372 Balmer epsilon (2-7) H+, He+ and Ar+ perturbers
(lambda = 3971.24, Kalpha = 2.948E-02)
tabl2-6 77 350 Balmer (2-8) H+ perturbers
(lambda = 3890.19, Kalpha = 4.302E-02)
tabl2-7 77 290 Balmer (2-9) H+ perturbers
(lambda = 3836.51, Kalpha = 6.190E-02)
tabl2-8 77 200 Balmer (2-10) H+ perturbers
(lambda = 3799.01, Kalpha = 8.344E-02)
tabl2-9 77 200 Balmer (2-2) H+ perturbers
(lambda = 3771.74, Kalpha = 1.094E-01)
tabl2-10 77 125 Balmer (2-12) H+ perturbers
(lambda = 3751.25, K = 1.407E-01)
tabl2-11 77 130 Balmer (2-13) H+ perturbers
(lambda = 3735.47, K = 1.774E-01)
tabl2-12 75 52 Balmer (2-14) H+ perturbers
(lambda = 3723.03, Kalpha = 2.202E-01)
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Byte-per-byte Description of file: tabl1-*
Byte-per-byte Description of file: tabl2-*
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Bytes Format Units Label Explanations
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1- 9 E9.2 cm-3 Ne Electron density
11- 19 E9.2 --- Delta Dlambda/Dalpha
21- 29 E9.2 K T Temperature
31- 39 E9.2 --- R0/Debye ratio of the mean interelectronic distance to
the electronic Debye length (1)
42- 50 E9.2 "alpha" Dalpha Detuning from line center (2), (3)
53- 61 E9.2 1/"alpha" IDH+ Intensity (with Doppler), H+ perturbers (3)
65- 73 E9.2 1/"alpha" ISH+ Intensity (Stark only), H+ perturbers (3)
79- 87 E9.2 1/"alpha" IDHe+ []? Intensity (with Doppler), He+ perturbers (3)
91- 99 E9.2 1/"alpha" ISHe+ []? Intensity (Stark only), He+ perturbers (3)
105-113 E9.2 1/"alpha" IDAr+ []? Intensity (with Doppler), Ar+ perturbers(3)
117-125 E9.2 1/"alpha" ISAr+ []? Intensity (Stark only), Ar+ perturbers (3)
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Note (1): R0/Debye is expressed in electrons
Note (2): Dalpha = (Delta lambda)/F0
where Delta lambda is the detuning, expressed in Angstroems
Note (3): The intensities are expressed in 1/alpha where
alpha= lambda0/F0,
lambda0 is the wavelength of the line center, in Angstroems
F0 is the normal Holstmark field strength value in ues units:
F0= 1.25 E-9 Ne**(2/3), Ne is the electronic density expressed in cm-3
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(End) Patricia Bauer [CDS] 04-Jan-1994