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J/ApJ/561/727       BVI photometry in the Antennae galaxies       (Zhang+, 2001)

A multiwavelength study of the young star clusters and interstellar medium in the Antennae galaxies. Zhang Q., Fall S.M., Whitmore B.C. <Astrophys. J. 561, 727 (2001)> =2001ApJ...561..727Z
ADC_Keywords: Galaxies, photometry Keywords: galaxies: individual (NGC 4038/9) - galaxies: interactions - galaxies: star clusters - stars: formation Abstract: We report on a multiwavelength study of the relationship between young star clusters in the Antennae galaxies (NGC 4038/9) and their interstellar environment, with the goal of understanding the formation and feedback effects of star clusters in merging galaxies. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 43 84 Red clusters in the Antennae galaxies
See also: J/AJ/109/960 : Young star clusters in The Antennae (Whitmore+ 1995) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 2 I2 --- [ZFW2001] Cluster number 4- 9 F6.2 arcsec oRA Right Ascension offset (1) 11- 16 F6.2 arcsec oDE Declination offset (1) 18 I1 --- Chip Chip number 20- 24 F5.2 mag VMAG The absolute V band magnitude 26- 29 F4.2 mag B-V ? The (B-V) color index 31- 34 F4.2 mag V-I The (V-I) color index 36- 39 F4.2 mag DelV1-6 The ΔV1-6 parameter (2) 41- 43 I3 --- [WS95] ? Whitmore & Schweizer (1995, Cat. J/AJ/109/960) number (3)
Note (1): Following the convention used in Whitmore & Schweizer (1995, Cat. J/AJ/109/960) and Whitmore et al. (1999AJ....118.1551W), the coordinates are the offsets from RA=12:01:52.97 and DE=-18:52:08.29 (J2000.0), near the center of NGC 4038. Note (2): The difference in V magnitudes measured in a 1-pixel and 6-pixel radius aperture, which provides a rough determination of cluster size. Objects with ΔV1-6<1.0 are likely to be cosmic rays. Note (3): Duplicated numbers are neighboring objects, generally because of differences in spatial resolution between the cycle 2 and cycle 5 observations.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Bauer [CDS] 14-Jan-2002
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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