J/ApJ/616/562        Rotational velocities in binaries              (Abt+, 2004)

Tidal effects in binaries of various periods. Abt H.A., Boonyarak C. <Astrophys. J., 616, 562-566 (2004)> =2004ApJ...616..562A 2004ApJ...616..562A
ADC_Keywords: Binaries, spectroscopic ; Stars, double and multiple ; Rotational velocities Keywords: binaries: spectroscopic - binaries: visual - stars: rotation Abstract: We found in the published literature the rotational velocities for 162 B0-B9.5, 151 A0-A5, and 86 A6-F0 stars, all of luminosity classes V or IV, that are in spectroscopic or visual binaries with known orbital elements. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 41 162 B0-B9.5 Dwarfs in Binaries table2.dat 39 151 A0-A5 Dwarfs in Binaries table3.dat 40 86 A6-F0 Dwarfs in Binaries -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat table2.dat table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- HR The HR designation number 5- 6 A2 --- m_HR Multiplicity index on HR 7 A1 --- l_vsini Limit flag on vsini 8- 11 I4 km/s vsini ? Primary projected velocity 12 A1 --- f_vsini [*] Indicates values from Bright Star Catalogue (1991, Cat. V/50) 14- 16 I3 km/s vsiniB ? Secondary projected velocity 19- 32 F14.6 d Per Period 34- 41 A8 --- Kind Binary type -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 17-May-2005
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