J/AJ/109/650                                          Arp 2 (Buonanno+ 1995)

Young Globular Clusters in the Milky Way: Arp 2 Buonanno R., Corsi C.E., Fusi Pecci F., Richer H.B., Fahlman G.G. <Astron. J. 109, 650 (1995)> =1995AJ....109..650B 1995AJ....109..650B
ADC_Keywords: Clusters, globular ; Photometry, CCD Abstract: We have obtained the first B,V CCD color-magnitude diagram (CMD) of the galactic globular cluster Arp 2. About 1600 stars have been measured between the tip of the red giant branch at V ∼ 15.5 and V ∼ 23.5, about two magnitudes below the main sequence turnoff. A centrally concentrated population of blue stragglers has been detected. The slope of the red giant branch and the overall CMD morphology are consistent with that of a metal-poor cluster, with [Fe/H] = 18.4±0.25. A preliminary spectroscopic measurement based on the Ca II triplet yields [Fe/H] = -1.73±0.05. The comparison of the CMD of Arp 2 with that of other clusters favors a value more metal-poor than that indicated by the Ca II triplet. In this respect, Arp 2 is similar to Ruprecht 106 [Buonanno et al. =1990AJ....100.1811B 1990AJ....100.1811B and =1993AJ....105..184B 1993AJ....105..184B]. Differential ages between Arp 2 and a number of reference clusters are obtained from the vertical age parameter Delta V^TO_HB, and the horizontal age parameter, Δ(B-V)^TO_RGB. By requiring both age estimators to give consistent results, we find that Arp 2 is ∼ 3 Gyr younger than the group of the metal-poor clusters and slightly older than Ruprecht 106. The detection of young metal-poor clusters ([Fe/H] ≤ -1.8) implies a complex scenario for the origin of the galactic halo, possibly involving interactions with satellite galaxies and their cluster systems. Objects: ------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------ 19 28 44 -30 21.5 Arp 2 = C 1925-304 ------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 28 1586 Magnitudes, colors, and positions of stars in the central field of Arp 2 table2.tex 100 965 TeX version of Table 2 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- Star Star number 5-12 F8.3 mag Vmag V magnitude 13-19 F7.3 mag B-V (B-V) color 20-24 I5 arcsec Xpos *X coordinate in local system 25-28 I4 arcsec Ypos *Y coordinate in local system -------------------------------------------------------------------------------- Note on Xpos, Ypos: X and Y coordinates in local system (hence, useful just for identification purposes) and are expressed in arcseconds relative to an arbitrary "center" adopted for the cluster. -------------------------------------------------------------------------------- Origin: AAS CD-ROM series, Volume 4, 1995 Lee Brotzman [ADS] 26-Apr-1995
(End) [CDS] 11-Jul-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