Results 21 to 30 of about 2,490 (267)
Missing for 20 yr: MeerKAT Redetects the Elusive Binary Pulsar M30B
PSR J2140−2311B is a 13 ms pulsar discovered in 2001 in a 7.8 hr Green Bank Telescope observation of the core-collapsed globular cluster M30 and predicted to be in a highly eccentric binary orbit.
Vishnu Balakrishnan +16 more
doaj +1 more source
New Parameters for Star Cluster Dynamics: The Effect of Primordial Binaries and Dark Remnants
By studying the normalized cumulative radial distribution (nCRD) of the stars in the central region of a Monte Carlo-simulated globular cluster, we recently defined three parameters able to pinpoint the stage of internal dynamical evolution reached by ...
B. Bhat +3 more
doaj +1 more source
Search for variable stars in globular clusters [PDF]
A program to search poorly studied southern globular clusters for variable stars is being carried out on the 1-m Yale telescope at CTIO. Recently two galactic bulge clusters of moderately high metallicity have been found to contain RR Lyrae variables; a cluster of similar metallicity a little farther from the galactic center apparently has none.
openaire +1 more source
Neutron Stars in Globular Clusters [PDF]
AbstractDynamical interactions that occur between objects in dense stellar systems are particularly important for the question of formation of X-ray binaries. We present results of numerical simulations of 70 globular clusters with different dynamical properties and a total stellar mass of 2×107M⊙.
Ivanova, Natalia +2 more
openaire +2 more sources
The Supersonic Project: Star Formation in Early Star Clusters without Dark Matter
The formation mechanism of globular clusters (GCs) has long been debated by astronomers. It was recently proposed that supersonically induced gas objects (SIGOs)–which formed in the early Universe due to the supersonic relative motion of baryons and dark
William Lake +9 more
doaj +1 more source
Star and Globular Cluster Formation in Mergers [PDF]
The high burst strengths and star formation efficiencies found with spectrophotmetric and chemical evolutionary synthesis for mergers of gas-rich spirals led us to expect the formation of a secondary population of globular clusters (GC) with enhanced metallicity (F. – v. A. & Gerhard 1994, A&A 285, 751 u.775).
openaire +2 more sources
THE SEQUENTIAL STAR FORMATION IN GLOBULAR CLUSTERS
The results of [O/Na] abundance modelling in globular clusters NGC 2808 and NGC 6752 are presented. The evolutionary scenario allowing to reproduce characteristic observed features of [O/Na] distribution function has been suggested.
M. V. Ryabova, Yu. A. Shchekinov
doaj +1 more source
Multiple Populations in Low-mass Globular Clusters: Eridanus
Multiple populations (MPs), characterized by variations in light elemental abundances, have been found in stellar clusters in the Milky Way, Magellanic Clouds, as well as several other dwarf galaxies.
Yue Wang +7 more
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The globular cluster migratory origin of nuclear star clusters [PDF]
19 pages, 20 figures, submitted to ...
ARCA SEDDA, MANUEL +1 more
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Variable stars in the globular cluster M 92 [PDF]
AbstractResults of a search for variable stars in the central region of the Oosterhoff II type globular cluster M92 are presented.
openaire +2 more sources

