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J/A+A/321/236       Reddening and fluxes of carbon stars    (Knapik+ 1997)

Interstellar extinction and the intrinsic spectral distribution of variable carbon stars Knapik A., Bergeat J. <Astron. Astrophys. 321, 236 (1997)> =1997A&A...321..236K (SIMBAD/NED BibCode)
ADC_Keywords: Stars, carbon ; Reddening ; Stars, variable Keywords: stars: AGB and post-AGB - stars: carbon - dust, extinction Description: This table contains our CV-classification (see Subsec. 3.3 in the paper) for 133 carbon variables and their colour excess E(B-V) as determined by the method described in Sec. 4. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3 37 133 CV-classification and colour excess of 133 carbon variables. table3.tex 70 154 LaTeX version of table3
See also: III/156 : General Catalog of Cool Galactic Carbon Stars, (Stephenson 1989) II/139 : General Catalog of Variable Stars, 4th Ed. (GCVS4) (Kholopov+ 1988) II/140 : New Catalogue of Suspected Variable Stars (Kukarkin+, 1982) II/125 : IRAS catalogue of Point Sources, Version 2.0 (IPAC 1986) J/A+A/342/773 : Hot carbon stars B-V colour excess. Paper II. (Bergeat+ 1999) J/A+A/344/263 : Miras B-V colour excess. Paper III. (Knapik+, 1999) J/A+A/369/178 : Eff. temp. of carbon-rich stars. Paper IV. (Bergeat+, 2001) Byte-by-byte Description of file: table3
Bytes Format Units Label Explanations
1- 4 I4 --- GCCS ? Stephenson's (1989) Cat. III/156 Catalogue entry 6- 15 A10 --- name GCVS or NSV or IRAS entry (1) 17- 22 F6.2 deg GLON Galactic longitude 24- 29 F6.2 deg GLAT Galactic latitude 31 I1 --- CV Carbon Variable classification (1 to 6) 33- 36 F4.2 mag E(B-V) Excess in the B-V colour index
Note (1): GCVS, General Catalogue of Variable Stars, Cat. II/139 NSV, New Suspected Variables, Cat. II/140 IRAS, IRAS Point Source Catalog, Cat. II/125
Acknowledgements: Jacques BERGEAT
(End) J. Bergeat CRAL-Observatoire de Lyon, Patricia Bauer [CDS] 25-Oct-1996
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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