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J/A+A/290/609       Be stars near-IR excess                   (Dougherty+, 1994)

Near-IR excess of Be stars DOUGHERTY S.M., WATERS L.B.F.M., BURKI G., COTE J., CRAMER N., VAN KERKWIJK M.H., TAYLOR A.R. <Astron. Astrophys. 290, 609 (1994)> =1994A&A...290..609D (SIMBAD/NED Reference)
ADC_Keywords: Stars, Be; Reddening Keywords: stars: emission-line, Be - infrared File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 83 144 Excess colours of 144 Be stars
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
2- 5 I4 --- HR []? HR number 7- 12 I6 --- HD HD number 15- 28 A14 --- Source Source name 30- 43 A14 --- Sp Spectral type (from the Bright Star Catalogue) 45- 49 F5.2 mag E[B-V]1 Excess [B-V] colour (calculated from spectral type) 51- 54 F4.2 mag E[B-V]2 []? Excess [B-V] colour from the 2175 angstrom interstellar absorption feature (Beeckmans and Hubert-Delplace (1980)) and converted using E(B-V) = 0.84E[B-V] (Cramer, 1984) 56- 60 F5.2 mag E[V-J] Excess [V-J] colour 62- 66 F5.2 mag E[V-H] []? Excess [V-H] colour 68- 72 F5.2 mag E[V-K] []? Excess [V-K] colour 74- 78 F5.2 mag E[V-L] []? excess [V-L] colour 80 A1 --- Ref Comment for the source of the observations: a) Dougherty et al., 1991 b) Dachs et al., 1988 c) Burki et al., in preparation Visual observations from Burki et al. (in preparation) except when n_Ref. = 5 82 A1 --- n_Ref If n_Ref = 5, the visual observations are taken from the catalogue of Rufener (1988)
References: Beeckmans, F., Hubert-Delplace, A.M. 1980, A&A 86, 72 Cramer, N. 1984, A&A 132, 283 Dachs, J., Engels, D., Kiehling, R. 1988, A&A 194, 167 Dougherty, S.M., Taylor, A.R., Clark, T.A. 1991a, AJ 102, 1753 Rufener, F. 1988, Catalogue of stars measured in the Geneva Observatory photometric system, 4th edn., Observatoire de Geneve
(End) Patricia Bauer [CDS] 30-May-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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