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J/A+A/499/827       Disk of υ Sgr                    (Netolicky+, 2009)

The circumbinary dusty disk around the hydrogen-deficient binary star υ Sagittarii. Netolicky M., Bonneau D., Chesneau O., Harmanec P., Koubsky P., Mourard D., Stee P. <Astron. Astrophys., 499, 827-833 (2009)> =2009A&A...499..827N (SIMBAD/NED BibCode)
ADC_Keywords: Stars, emission Keywords: stars: emission-line, Be - stars: binaries: close - stars: circumstellar matter - techniques: interferometric - stars: individual: upsilon Sagittarii Abstract: The aim of this paper is to determine the properties of the dusty environment of the hydrogen-deficient binary system upsilon Sgr, whose binary properties and other characteristics are poorly known. We obtained the first mid-IR interferometric observations of upsilon Sgr using the instrument MIDI of the VLTI used with different pairs of 1.8m and 8m telescopes. The calibrated visibilities, the N band spectrum, and the SED were compared with disk models computed with the MC3D code to determine the geometry and chemical composition of the envelope. ************************************************************************** * * * Sorry, but the author(s) never supplied the tabular material * * announced in the paper * * * ************************************************************************** File Summary:
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ReadMe 80 . This file
Author's address: M. Netolicky,
(End) Patricia Vannier [CDS] 04-Jan-2010
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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