Photometry of the globular cluster M54 and the Sagittarius dwarf galaxy: The age-metallicity relation

AC Layden, A Sarajedini - The Astronomical Journal, 2000 - iopscience.iop.org
We present deep VI-band photometry of the globular cluster M54, a nearby field in the
Sagittarius dwarf galaxy, and a control field. The color-magnitude diagrams reach well …

The ACS Virgo Cluster Survey. XIV. Analysis of color-magnitude relations in globular cluster systems

S Mieske, A Jordán, P Côté… - The Astrophysical …, 2006 - iopscience.iop.org
We examine the correlation between globular cluster (GC) color and magnitude using HST
ACS imaging for a sample of 79 early-type galaxies (-21.7< MB<-15.2 mag) with accurate …

VLT-UVES analysis of two giants in the bulge metal-poor globular cluster HP-1-Analysis of two giants in HP-1

B Barbuy, M Zoccali, S Ortolani, Y Momany… - Astronomy & …, 2006 - aanda.org
Context. Metal-poor globular clusters in the bulge are important tracers of early chemical
evolution. HP-1 is among the six metal-poor clusters within 5° of the Galactic center, and …

VI photometry of the post-core-collapse globular cluster NGC 6558 and the adjacent bulge field population

RM Rich, S Ortolani, E Bica… - The Astronomical Journal, 1998 - iopscience.iop.org
We present VI color-magnitude diagrams (CMDs) of the globular cluster NGC 6558 and its
surrounding field, obtaining cluster parameters. The cluster has a blue extended horizontal …

HST observations of Terzan 1: a second parameter globular cluster in the galactic bulge

S Ortolani, B Barbuy, ELD Bica, A Renzini… - … . Berlin. Vol. 350, no. 3 …, 1999 - lume.ufrgs.br
Hubble Space Telescope observations in the F555W and F814W bands are presented of
the bulge globular cluster Terzan 1. This highly obscured cluster has the smallest projected …

Integrated spectral study of reddened globular clusters and candidates

E Bica, JJ Claria, AE Piatti, C Bonatto - Astronomy and Astrophysics …, 1998 - aas.aanda.org
This paper presents integrated spectra in the range 6700-9500 for 20 Galactic globular
clusters (and candidates) in the bulge and 5 others projected on the Galactic disk (and) …

Spectroscopic analysis of the candidate globular clusters NGC 1928 and 1939 in the Large Magellanic Cloud

CM Dutra, E Bica, JJ Clariá… - Monthly Notices of the …, 1999 - academic.oup.com
The integrated spectral properties in the range 3600–6700 Å of the candidate old clusters
NGC 1928 and 1939 in the LMC bar are compared with those of old-and intermediate-age …

Update on Pulsar B162026 in M4: Observations, Models, and Implications

S Sigurdsson, SE Thorsett - arXiv preprint astro-ph/0404538, 2004 - arxiv.org
The combination of ever more precise radio timing data and serendipitous {\it HST} data has
confirmed that the outer companion to PSR B1620 $-$26 is a planet. Here we summarize …

Gravitational interactions between globular and open clusters: an introduction

R De la Fuente Marcos, C De la Fuente Marcos… - Astrophysics and Space …, 2014 - Springer
Historically, it has been assumed that globular and open clusters never interact. However,
recent evidence suggests that: globular clusters passing through the disk may be able to …

Placing the Fornax and Sagittarius dwarf spheroidal globular clusters in the horizontal-branch type versus metallicity diagram

EO Smith, RM Rich, JD Neill - The Astronomical Journal, 1998 - iopscience.iop.org
We plot the globular clusters of the Fornax galaxy and those associated with the Sagittarius
dwarf spheroidal galaxy in the horizontal-branch type versus metallicity diagram. The …