Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...331...70g&link_type=abstract
Astronomy and Astrophysics, v.331, p.70-80 (1998)
Astronomy and Astrophysics
Astrophysics
60
Globular Clusters: Ngc6553, Galaxy: Center, Blue Stragglers, Hr Diagram
Scientific paper
JK infrared photometry for the bulge globular cluster NGC 6553, combined with high resolution visual VI observations are presented and discussed in connection with the bulge metal rich population. The infrared data were taken with IRAC2 at ESO 2.2m telescope while the optical counterparts are from Hubble Space Telescope (HST). We find a mean magnitude for the horizontal branch of VHB =3D 16.92, and KHB =3D 12.42 +/- 0.01. Assuming a reddening of E(B-V)=3D 0.7, the mean distance modulus is (m-M)_0 =3D 13.6 giving an heliocentric distance of 5.2Kpc. This distance is slightly higher than that previously published by Ortolani et al. (1990, hereafter OBB90). The brightest giants have been detected at K ~ 6.5 and (V-K) =3D 13.10 transforming to M_K =3D -7.34 and (V-K){_0} =3D 11.20, which are exceptionally high values for a globular cluster. The metallicity has been found to be consistent with previous values and an average of [Fe/H] =3D -0.22 +/- 0.05 has been adopted. The helium abundance estimated via the R' method yields Y_p ~ 0.28 +/- 0.03. Based on observations obtained at ESO-La Silla, Chile and with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, operated by AURA Inc. under contract to NASA.\hfill\break Appendix only available in electronic form at the CDS (Strasbourg) via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html
Barbuy Batriz
Bica Eduardo
Guarnieri Maria Donata
Moneti Andrea
Montegriffo Paolo
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