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J/A+AS/113/35       Rotation curves of galaxies in DC 1842-63     (Amram+, 1995)

H α velocity fields and rotation curves of galaxies in clusters. III. Nine galaxies in DC 1842-63 AMRAM P., BOULESTEIX J., MARCELIN M., BALKOWSKI C., CAYATTE V., SULLIVAN W.T.III <Astron. Astrophys. Suppl. Ser. 113, 35 (1995)> =1995A&AS..113...35A (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, galaxy; Radial velocities Keywords: galaxies: kinematics and dynamics - galaxies: clusters - galaxies: ISM - galaxies: clusters: DC 1842-63 Description: H α maps, velocity contour maps and rotation curves are presented for nine galaxies in the Southern cluster DC 1842-63. These data have been obtained from the two-dimensional H α observations at the 3.60m ESO Telescope equipped with CIGALE, a scanning Fabry-Perot interferometer. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table3 74 85 Detailed information about the rotation curves
Byte-by-byte Description of file: table3
Bytes Format Units Label Explanations
1- 4 A4 --- Galaxy Galaxy 6- 9 F4.1 arcsec R Mean radius on the major axis of the annulus for which the rotational velocity is calculated 14- 16 I3 --- Napp Number of points with measurable velocities in the annulus for the approaching side of the galaxy 21- 23 I3 km/s Vapp []? Weighted average velocity calculated from the Napp points 33- 34 I2 km/s e_Vapp []?Error in Vapp (± r.m.s.) 39- 41 I3 --- Nrec Number of points with measurable velocities in the annulus for the receding side 46- 48 I3 km/s Vrec []? Weighted average velocity calculated from the Nrec points 58- 59 I2 km/s e_Vrec []? Error in Vrec (± r.m.s.) 61- 63 I3 --- Ntot Total number of velocity points N=Napp+Nrec 65- 67 I3 km/s Vtot Weighted average velocity computed from both sides 73- 74 I2 km/s e_Vtot Error in Vtot (± r.m.s.)

(End) Simona Mei [CDS] 13-Apr-1995
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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