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J/A+A/326/249       Chromospheric models of dwarf M stars (Mauas+ 1997)

Chromospheric models of dwarf M stars Mauas P., Falchi A., Pasquini L., Pallavicini R. <Astron. Astrophys. 326, 249 (1997)> =1997A&A...326..249M
ADC_Keywords: Stars, M-type ; Models, atmosphere Keywords: stars: atmospheres - stars: chromospheres - stars: late-type - Description: Tables 4 and 5 give the atmospheric parameters for our models of dM stars Gl 588 and Gl 628. The columns give the column mass in g/cm-2, the electron temperature in K, the microturbulent velocity in km/s; the continuum optical depth at 5000Å; the hydrogen, proton, and electron density in particles per cm-3; and the height h (in km) above the level where tau5000=1. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 15 32 18 -41 15 42 Gl 588 16 30 18 -12 38 47 Gl 628 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table4 62 41 Atmospheric parameters for our model for Gl 588 table5 62 41 Atmospheric parameters for our model for Gl 628 tables.tex 81 143 TeX version of the tables
Byte-by-byte Description of file: table4 table5
Bytes Format Units Label Explanations
1- 9 E9.3 g/cm2 Mass Column mass 11- 16 I6 K Te Electron temperature 18- 21 F4.2 km/s Vtur Microturbulent velocity 23- 30 E8.2 --- tau5000 Continuum optical depth at 5000Å (500nm) 32- 39 E8.2 cm-3 NH Hydrogen density 41- 48 E8.2 cm-3 Np Proton density 50- 57 E8.2 cm-3 Ne Electron density 59- 62 I4 km h Height above the level where tau5000Å=1
Acknowledgements: Ambretta Falchi
(End) A. Falchi [Osservatorio di Arcetri], Patricia Bauer [CDS] 10-Apr-1997
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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