J/A+A/352/297       The dust content of planetary nebulae   (Stasinska+, 1999)

The dust content of planetary nebulae: a reappraisal Stasinska G., Szczerba R. <Astron. Astrophys. 352, 297 (1999)> =1999A&A...352..297S 1999A&A...352..297S (SIMBAD/NED BibCode)
ADC_Keywords: Planetary nebulae ; Reddening Keywords: planetary nebulae: general - infrared: stars - stars: AGB and post-AGB - stars: circumstellar matter - radiative transfer Description: This table contains the dust temperatures and dust-to-gas mass ratios derived for a sample of planetary nebulae and the observational data used for these determinations File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 77 548 Observational and derived data for the analysed sample of planetary nebulae -------------------------------------------------------------------------------- See also: V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+, 1992) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 11 A10 --- PNG PNG identification of planetary nebula 15- 26 A12 --- Name Ususal planetary nebula name 31- 39 E9.2 mW/m+2 F(Hbeta) ? Reddening corrected nebular Hbeta flux 42- 47 F6.2 arcsec theta ? Angular radius of nebula 50- 58 E9.2 cm-3 Ne ? Electron density 62- 66 F5.0 K Td Derived dust temperature 68- 77 E10.2 --- Md/Mg ? Derived dust-to-gas mass ratio -------------------------------------------------------------------------------- Acknowledgements: Ryszard Szczerba
(End) Patricia Bauer [CDS] 23-Nov-1999
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