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J/A+AS/135/145      HII region catalogue of NGC 7479         (Rozas+, 1999)

Global properties of the population of HII regions in NGC 7479 from photometric Hα imaging. Rozas, M. Zurita, A., Heller, C. H., Beckman, J. E. <Astron. Astrophys. Suppl. Ser. 135, 145 (1999)> =1999A&AS..135..145R
ADC_Keywords: H II regions ; Galaxies, optical Keywords: ISM: HII regions - galaxies: individual: NGC 7479 - galaxies: spiral Description: HII region catalogue of the barred galaxy NGC 7479. The catalogue contains the position, mean radius and the calibrated H-alpha luminosity of each HII region. The HII region catalogue has been composed using a new semi-automated technique applied to a high quality continuum-subtracted H-alpha image of the galaxy obtained from observations through the TAURUS camera in imaging mode with the 4.2m WHT on La Palma. An EEV CCD 7 detector was used with a projected pixel size of 0.279". More details about the reduction and the catalogue production procedures are given in the paper. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file catalog.dat 48 1009 The HII region catalogue of NGC 7479
See also: J/A+A/354/823 : HII region catalogue of NGC 3359 (Rozas+, 2000) Byte-by-byte Description of file: catalog.dat
Bytes Format Units Label Explanations
1- 4 I4 --- [RZH99] [1,1009]+ Identification number 8- 14 F7.2 arcsec oRA Right ascension of each HII region with respect to the centre (positive offsets toward the E) (1) 19- 25 F7.2 arcsec oDE Declination of each HII region with respect to the centre (positive offsets toward the N) (1) 32- 38 F7.4 [10-7W] logLHa Decimal logarithm of the Hα luminosity 45- 48 F4.2 arcsec radius Radius of HII region
Note (1): The centre of the galaxy is RA = 23h 04m 57.1s, DE = 12° 19' 18" (2000)
Acknowledgements: Almudena Zurita Munoz
(End) Patricia Bauer [CDS] 08-Feb-2001
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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