J/A+AS/137/233      UBVI imaging photometry of NGC 6231 (Baume+, 1999)

UBVI imaging photometry of NGC 6231 Baume G., Vazquez R.A., Feinstein A. <Astron. Astrophys. Suppl. Ser. 137, 233 (1999)> =1999A&AS..137..233B 1999A&AS..137..233B (SIMBAD/NED BibCode)
ADC_Keywords: Photometry, UBVRI ; Clusters, open Keywords: cluster: open - individual: Cr 272 - stars: luminosity function, mass function - HR diagram Description: CCD UBVI photometry in the field of the open cluster NGC 6231 was obtained for 1060 stars down to V=19mag. Memberships, reddening, distance and age of this cluster were investigated. Its lower sequence displays a notorious bend at V=13.5mag followed by a high number of faint stars showing a large magnitude spread at constant colour. This distribution of stars does not seem to be produced by a mere accumulation of field stars seen in the direction of the cluster but by a real star excess in the zone. The evidence suggests these stars are serious candidates to be cluster members caught in their way towards the ZAMS. Fitting them with pre main sequence isochrones an age spread of 10Myr is obtained. The luminosity and mass functions were found to be flat for -7.5<Mv<1.5 and for 3 to 80M respectively. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 16 54 12 -41 48.0 NGC 6231 = C 1650-417 ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 64 1050 CCD photometric observations in NGC 6231 table1.tex 111 793 LaTeX version of Table 1 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- Seq Sequence number 9- 14 F6.1 pix Xpos X position (1) 17- 22 F6.1 pix Ypos Y position (1) 26- 30 F5.2 mag Vmag V magnitude 31- 32 A2 --- u_Vmag [: ] Uncertainty flag on Vmag (2) 34- 38 F5.2 mag B-V B-V colour index 39- 40 A2 --- u_B-V [: ] Uncertainty flag on B-V (2) 42- 46 F5.2 mag U-B ? U-B colour index 47- 48 A2 --- u_U-B [: ] Uncertainty flag on V-R (2) 50- 54 F5.2 mag V-I ? V-I colour index 55- 56 A2 --- u_V-I [: ] Uncertainty flag on V-I (2) 58- 61 A4 --- Rem Remarks (3) -------------------------------------------------------------------------------- Note (1): 1 pix = 0.45". X increases from East to West, Y increases from South to North Note (2): (:) errors from 0.10 to 0.20 (::) errors larger than 0.20 Note (3): lm: likely member nm: non member pm: probable member 1: suspected variable in view of the photometric differences between our data and the Perry et al. (1991A&AS...90..195P 1991A&AS...90..195P, PHC) ones. ΔV in relation to PHC V mag are: # 13 = -0.16 # 38 = -0.18 (Also probable β Cep according to PHC) # 41 = 0.13 # 69 = -0.17 # 72 = -0.12 # 148 = -0.12 # 153 = -0.15 # 166 = -0.16 (Also probable variable according to PHC) # 169 = -0.11 2: variable star according to Balona & Laney (1995MNRAS.276..627B 1995MNRAS.276..627B) 3: variable according to Feinstein & Ferrer (1968PASP...80..410F 1968PASP...80..410F) and Raboud et al. (1997, Cat. J/A+A/325/167) 4: β Cep according to Balona & Laney (1995MNRAS.276..627B 1995MNRAS.276..627B) -------------------------------------------------------------------------------- Acknowledgements: Gustavo L. Baume
(End) Gustavo L. Baume [Observ. Astron. La Plata] 01-Jun-1999
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