Dynamics of star clusters/ by International Astronomical Union Symposium (113th : 1984 : Princeton, New Jersey), Goodman, Jeremy, Hut, Piet

On Encounter Rates in Star Clusters by Krisada Rawiraswattana, Simon P. Goodwin

Subjects: “…Star clusters…”
Get full text

Multiple Populations in Star Clusters by Antonino P. Milone, Anna F. Marino

Get full text

Star clusters and how to observe them / by 224414 Allison, Mark

New atlas of open star clusters by Seleznev Anton F., Avvakumova Ekaterina, Kulesh Maxim, Filina Julia, Tsaregorodtseva Polina, Kvashnina Alvira

“…Due to numerous new discoveries of open star clusters in the last two decades, astronomers need an easy-touse resource to get visual information on the relative position of clusters in the sky. …”
Get full text

Super-resolving star clusters with sheaves by Michael Robinson, Christopher T. Capraro

Subjects: “…Star cluster…”
Get full text

Nuclear Star Clusters and Black Holes by Seth, A, Cappellari, M, Neumayer, N, Caldwell, N, Bastian, N, Olsen, K, Blum, R, Debattista, V, McDermid, R, Puzia, T, Stephens, A

“…We summarize the recent results of our survey of the nearest nuclear star clusters. The purpose of the survey is to understand nuclear star cluster formation mechanisms and constrain the presence of black holes using adaptive optics assisted integral field spectroscopy, optical spectroscopy, and HST imaging in 13 galaxies within 5 Mpc. …”

Star cluster parameters without isochrones by Wilson, R

“…An algorithm for objective Least Squares solution of star cluster HR diagrams (HRDs) is outlined, stimulated by the limited usefulness of 1-dimensional isochrones. …”

Structural Parameters of Star Clusters: Stochastic Effects by Narbutis D., Stonkutė R., de Meulenaer P., Mineikis T., Vansevičius V.

Subjects: “…galaxies: star clusters: general…”
Get full text

Fractal origin of the ideal hierarchical star clusters by V. G. Surdin

“…Perhaps this is a reason why formation of hierarchical star clusters take place very rare.…”
Get full text

Does God play dice with star clusters? by Michael Y. Grudic, Stella S.R. Offner, Dávid Guszejnov, Claude-André Faucher-Giguère, Philip F. Hopkins

Get full text

Kernel Density Estimation in the Study of Star Clusters by Seleznev Anton F.

“…The kernel estimator method is used to evaluate the surface and spatial star number density in star clusters. Both density maps and radial density profiles are plotted. …”
Get full text

IFS and IR observations of star clusters in the Antennae by Mengel, S, Lehnert, MD, Thatte, N, Genzel, R

“…We find that all of the bright star clusters are young (< 20 Myrs), but the "overlap region" hosts the youngest clusters (similar to5 Myrs), while the nuclear starbursts started similar to100 Myrs ago. …”

Structural Parameters of Star Clusters: Signal to Noise Effects by Narbutis D., Bridžius A., Semionov D.

Subjects: “…galaxies: star clusters: general…”
Get full text

Stochasticity in Star Clusters: Reduced Random Sampling Method by de Meulenaer P., Narbutis D., Mineikis T., Vansevičius V.

Subjects: “…galaxies: star clusters: general…”
Get full text

A Young Star Cluster in the Leo a Galaxy by Stonkutė R., Narbutis D., Bridžius A., Leščinskaitė A., Vansevičius V.

Subjects: Get full text

On the density and surface brightness profiles in globular star clusters by Ninković S., Valjarević A.

“…A model of mass distribution, applicable to globular star clusters and proposed earlier, is reconsidered. …”
Get full text

Collisional Shaping of Nuclear Star Cluster Density Profiles by Sanaea C. Rose, Morgan MacLeod

Subjects: Get full text

Stirred, not shaken: star cluster survival in the slingshot scenario by Carrillo, DRM, Fellhauer, M, Boekholt, TCN, Stutz, A, Inostroza, MCBM

“…Motivated by recent observational constraints, we model the host gas filament as a cylindrically symmetrical potential, and the star cluster as a Plummer sphere. In the model, the motion of the filament will produce star ejections from the cluster, leaving star cluster remnants that can be classified into four categories: (a) filament-associated clusters, which retain most of their particles (stars) inside the cluster and inside the filament; (b) destroyed clusters, where almost no stars are left inside the filament, and there is no surviving bound cluster; (c) ejected clusters, that leave almost no particles in the filament, since the cluster leaves the gas filament; and (d) transition clusters, corresponding to those clusters that remain in the filament, but that lose a significant fraction of particles due to ejections induced by filament oscillation. …”

Dynamical masses of young star clusters in interacting galaxies by Mengel, S, Lehnert, MD, Thatte, N, Genzel, R

“…Using ISAAC on VLT-ANTU and UVES on VLT-KUEYEN we have begun a program to measure stellar velocity dispersions of young star clusters in merging and interacting galaxies. In this contribution, we present results for clusters in two interacting galaxies - NGC 4038/39 and NGC 1487. …”