J/A+AS/119/191      CCD BVI photometry in NGC 5927 (Samus+, 1996)

A CCD BVI color-magnitude study of the metal-rich globular cluster NGC 5927 Samus N., Kravtsov V., Ipatov A., Smirnov O., Alcaino G., Liller W., Alvarado F. <Astron. Astrophys. Suppl. Ser. 119, 191 (1996)> =1996A&AS..119..191S 1996A&AS..119..191S (SIMBAD/NED BibCode)
ADC_Keywords: Clusters, globular ; Photometry, CCD Keywords: globular clusters: individual: NGC 5927 - HR diagram Description: We present for the globular cluster NGC 5927 the first multicolor CCD photometry that reaches below the cluster's main sequence turnoff. The turnoff is located approximately at VTO=20.1mag, (B-V)TO=1.18mag, (V-I)TO=1.30mag. There is a hint of horizontal branch morphology variations with distance from the cluster center. Using the isochrones of VandenBerg & Bell (1985ApJS...58..561V 1985ApJS...58..561V), we derive the cluster age to be about 15Gyr. Objects: ---------------------------------------------- RA (2000) DE Name ---------------------------------------------- 15 27 41 -50 39.5 NGC 5927 ---------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3 41 4136 CCD photometry in NGC 5927 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3 -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 5 I4 --- No [1/4136] Running number 7- 13 F7.3 pix Xpos X coordinate (1) 15- 21 F7.3 pix Ypos Y coordinate (1) 23- 28 F6.3 mag Vmag V magnitude 30- 34 F5.3 mag B-V ? B-V color 36- 41 F6.3 mag V-I ? V-I color -------------------------------------------------------------------------------- Note (1): X coordinate is along right ascension and increases from West to East, Y coordinate is along declination and increases from North to South. -------------------------------------------------------------------------------- Courtesy: Nikolai N. Samus,
(End) Patricia Bauer [CDS] 12-Apr-1996
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