Results 21 to 30 of about 102,398 (346)

Globular cluster candidates within the Fornax Cluster: Intracluster globulars? [PDF]

open access: yesAstronomy & Astrophysics, 2003
We present the results of a search for globular clusters in the surroundings of 15 low surface brightness dwarf galaxies belonging to the Fornax Cluster, which was carried out on CCD images obtained with the C and T1 filters of the Washington photometric system.
Boris Dirsch   +5 more
openaire   +4 more sources

Intergalactic Globular Clusters [PDF]

open access: yesHighlights of Astronomy, 2005
AbstractWe confirm and extend our previous detection of a population of intergalactic globular clusters in Abell 1185, and report the first discovery of an intergalactic globular cluster in the nearby Virgo cluster of galaxies. The numbers, colors and luminosities of these objects can place constraints on their origin, which in turn may yield new ...
Nial R. Tanvir   +7 more
openaire   +3 more sources

THE FLATTENING OF GLOBULAR CLUSTERS [PDF]

open access: yesThe Astronomical Journal, 1983
In the three nearest luminous galaxies, the Milky Way System, the Andromeda Galaxy and NGC 5128 the brightest globular clusters are rounder than the faintest ones. On the other hand (contrary to some previous results) the flattening of individual LMC clusters is found to be independent of their luminosities.
openaire   +5 more sources

Globular cluster formation in the Virgo cluster [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
Metal poor globular clusters (MPGCs) are a unique probe of the early universe, in particular the reionization era. Systems of globular clusters in galaxy clusters are particularly interesting as it is in the progenitors of galaxy clusters that the earliest reionizing sources first formed. Although the exact physical origin of globular clusters is still
Moran C. Corbett, Teyssier R., Lake G.
openaire   +3 more sources

THE ABUNDANCES IN THE STELLAR ATMOSPHERES IN THE M13 GLOBULAR CLUSTER

open access: yesOdessa Astronomical Publications, 2017
The chemical composition of 5 stars' atmospheres in globular cluster M13 and 2 halo stars taken from literature have been computed. A slight excess of O and deficit of Mg have been defined for globular cluster stars.
T. V. Mishenina, S. V. Kutsenko
doaj   +1 more source

Dynamical Substructures of Galactic Globular Clusters I. M5 [PDF]

open access: yesJournal of Astronomy and Space Sciences, 2004
CCD images to study the dynamical substructure of the globular cluster M5. We investigate the radial variation of ellipticities and position angles using the stellar photometry and the IRAF ellipse task.
Jongwhan Rhee, Young-Jong Sohn
doaj   +1 more source

Extragalactic Globular Clusters in the Near-Infrared: V. IC 4051 and NGC 3311 [PDF]

open access: yes, 2005
We present the results of combined optical and near-infrared photometry for the globular cluster systems of the giant ellipticals IC 4051 and NGC 3311.
Barmby   +62 more
core   +1 more source

Calibrating X-Ray Binary Luminosity Functions via Optical Reconnaissance. II. The High-mass XLF and Globular Cluster Population of X-Ray Binaries in the Low Star-forming Spiral M81

open access: yesThe Astrophysical Journal, 2023
We characterize the optical counterparts to the compact X-ray source population within the nearby spiral galaxy M81 using multiband Hubble Space Telescope (HST) imaging data.
Qiana Hunt   +4 more
doaj   +1 more source

Extragalactic Globular Clusters in the Near-Infrared II. The Globular Clusters Systems of NGC 3115 and NGC 4365 [PDF]

open access: yes, 2002
We combine near-infrared photometry obtained with the VLT/ISAAC instrument and archival HST/WFPC2 optical images to determine VIK magnitudes and colours of globular clusters in two early-type galaxies, NGC 3115 and NGC 4365.
Brodie, J. P.   +7 more
core   +5 more sources

The youngest globular clusters [PDF]

open access: yesInternational Journal of Modern Physics D, 2014
It is likely that all stars are born in clusters, but most clusters are not bound and disperse. None of the many protoclusters in our Galaxy are likely to develop into long-lived bound clusters. The super star clusters (SSCs) seen in starburst galaxies are more massive and compact and have better chances of survival. The birth and early development of
openaire   +3 more sources

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