VI/57 Radii of Be star line emitting regions (Jaschek+ 1993)
Catalogue of Radii of Be star Line Emitting Regions
Jaschek C., Jaschek M.
<Astron. Astrophys. Suppl. Ser. 97, 807 (1993)>
=1993A&AS...97..807J 1993A&AS...97..807J
ADC_Keywords: Stars, Be ; Stars, diameters
Description:
This bibliographic catalogue lists radii of line emitting regions
around more than 100 Be stars determined from high signal to noise
registrations of emission line profiles, listed in nine papers.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 59 636 Observational data and radii of the emission-
line forming regions.
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Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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2- 8 A7 --- HD HD number of the star (Cat. III/135)
12- 15 A4 --- HR HR number if it exists (Cat. V/50)
18- 20 I3 km/s peak Mesured separation of the emission line peaks.
21 A1 --- u_peak [:)] insecure peak values (1)
24- 28 I5 0.1nm lambda wavelength (in Angstrom) of the line used (2)
31- 38 A8 "DD.MM.YY" ObsDate Observing date (day, month, year-1900)
41- 43 I3 km/s vsini ? Rotational velocity as given by the author
46 I1 --- r_vsini bibliographic code (3)
48- 52 F5.2 --- R1 ? Radius of the line emitting region in units
of the stars radius (4)
53 A1 --- u_R1 [)] insecure R1 value (1)
55- 59 F5.1 --- R2 ? squared radius of the line emitting region
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Note (1):
Parentheses stand for uncertain values, blanks for either cases in
which the Vsin i values is non-existent or for those physically
impossible cases R < 1.
Note (2): Identification of the lines (table 3 of the paper):
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---- Wavelength ---- Multiplet
Observed Laboratory
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10048 10049.38 H P7
8750 8750.47 H P12
8598 8598.39 H P13
8467 8467.26 H P14
8446 8446.35+46.76 OI M.4
7772 7771.96+74.18+75.40 OI M.1
7712 7711.71 FeII M.73
6562 6562.82 H H3
6516 6516.05 FeII M.40
6384 6383.75 FeII
6371 6371.36 SiII M.2
5317 5316.61 FeII M.49
5169 5169.03 FeII M.42
4861 4861.33 H H4
4584 4583.83 FeII M.38
4340 4340.47 H H5
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Note (3): References (table 2 of paper)
1 - Andrillat Y., Jaschek M., and Jaschek C. 1990A&AS...84...11A 1990A&AS...84...11A
(table XII)
2 - Andrillat Y., Jaschek M., and Jaschek C. 1990A&AS...85..855A 1990A&AS...85..855A
(table III)
3 - Andrillat Y. 1983A&AS...53..319A 1983A&AS...53..319A (table I)
4 - Hanuschik R.W. 1986A&A...166..185H 1986A&A...166..185H (radii derived from table 1)
5 - Hanuschik R.W. 1987A&A...173..299H 1987A&A...173..299H (radii derived from table 3)
6 - Hanuschik R.W., Kozok J.R., and Kaiser D. 1988A&A...189..147H 1988A&A...189..147H
(radii derived from table 3)
7 - Slettebak A. 1992 ApJ in press (1994ApJS...94..163S 1994ApJS...94..163S)
8 - Jaschek M., Andrillat Y., and Jaschek C. 1993A&AS...97..781J 1993A&AS...97..781J
(table 7)
9 - Dachs J., Hummel W., and Hanuschik R.W. 1992A&AS...95..437D 1992A&AS...95..437D
(radii derived from tables 2, 3 and 4)
Note (4): radius derived by means of:
2 V sin i
R = ---------
ΔE
where ΔE represents the peak separation of the emissions.
The uncertainties are of the order of 20%.
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History:
* 17-Jul-1993: Original version
* 15-May-2004: ReadMe standardized
(End) Francois Ochsenbein [CDS] 15-May-2004