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J/PASP/98/1133      The open cluster NGC 346                    (Niemela+, 1986)

The young open cluster NGC 346 in the Small Magellanic Cloud NIEMELA V.S., MARRACO H.G, CABANNE M.L. <Publ. Astron. Soc. Pac. 98, 1133 (1986)> =1986PASP...98.1133N (SIMBAD/NED Reference)
ADC_Keywords: Magellanic Clouds; Clusters, open; Photometry, CCD Keywords: open cluster - CCD photometry - radial velocities - O-type stars Abstract: We present CCD photometry and spectrographic observations for stars in the open cluster NGC 346, which excites the largest H II region in the Small Magellanic Cloud. These observations show that NGC 346 is an extremely young cluster, containing more than 20 hot O-type stars. A radial-velocity study of the brightest stars, and also of the nearby supergiant Of star Sk 80, discloses atmospheric expansion due to strong stellar winds, but no large-amplitude radial-velocity variations due to short-period binary motion. However, two stars are probably longer period binaries. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 31 58 NGC 346 VRI (Kron-Cousins) CCD photometry
Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
1- 2 I2 --- Id Star number 9- 13 F5.2 mag Vmag V magnitude 16- 20 F5.2 mag V-R V-R colour index 23- 27 F5.2 mag V-I V-I colour index 31 I1 --- Rem [1-6]? Remarks (1)
Note (1): 1: integrated magnitude of a double star, not in Figure 3 and 4. 2: data correspond only to the brightest member of the group. 3: V observation affected by a cosmic ray, not in Figures 3 and 4. 4: red star, not in Figure 4. 5: integrated magnitude of a double star. 6: probably non-member, far from cluster center, not in Figure 4.
Table2 : Spectral classification and absolute magnitudes of the brightest stars in NGC 346 ----------------------------------------------------------------------------- Star Spectral Source Mv Remarks Type ----------------------------------------------------------------------------- 25 O8.5 III a,c -6.6 No. 2 in a 26 O4 III(f) a -7.1 No. 1 in a 28 O5-6: V: c -5.4 Only 1 weak spectrum 29 O3 III(f) b,c -6.1 No. 3 in b 30 O5-6 V b,c -5.9 No. 4 in b 32 O4-5 V c -5.5 ----------------------------------------------------------------------------- a: Walborn N.R., 1978, Ap.J. (Letters), 224, L133 b: Walborn N. R. and Blades J.C., 1986, Ap.J. (Letters), 304, L17 c: This study. Historical Notes: Keupunched at CDS
(End) Marie-Jose Wagner, Patricia Bauer [CDS] 02-Mar-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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