UOCS XIV: Study of the Open Cluster NGC 2627 Using UVIT/AstroSat
We study the intermediate-age open cluster NGC 2627, located at a distance of ∼2 kpc, using UVIT/AstroSat and other archival data. Using a machine learning-based algorithm, ML-MOC, on the Gaia DR3 data, we identify 422 cluster members, including four ...
Pinapati Saketh +2 more
doaj +1 more source
Cracking the Relation between Mass and 1P Star Fraction of Globular Clusters. I. Present-day Cluster Masses as a First Tool [PDF]
G. Parmentier
openalex +1 more source
Stellar-mass black holes in star clusters: implications for gravitational-wave radiation [PDF]
Sambaran Banerjee +2 more
openalex +1 more source
Formation Process of the Young Stellar Population in Messier 16 from a Kinematic Perspective
We present a kinematic study of young stars in Messier 16 (M16) using the Gaia Data Release 3 and high-resolution spectra. A total of 345 stars are selected as genuine members using the published lists of X-ray sources, infrared sources, and early-type ...
Beomdu Lim +6 more
doaj +1 more source
Open Cluster Study Using Gaia. I. Membership and Cluster Properties
Star clusters are interesting laboratories to study star formation, single and binary stellar evolution, and stellar dynamics. We have used the exquisite data from Gaia’s Data Release 3 (DR3) to study 21 relatively rich and nearby open clusters with ...
Anindya Ganguly +2 more
doaj +1 more source
Whole-sequence analysis indicates that the Y chromosome C2*-Star Cluster traces back to ordinary Mongols, rather than Genghis Khan. [PDF]
Wei LH +13 more
europepmc +1 more source
The life cycle of star clusters in a tidal field [PDF]
Mark Gieles +2 more
openalex +1 more source
A WISE Survey of New Star Clusters in the Central Plane Region of the Milky Way [PDF]
Jinhyuk Ryu, Myung Gyoon Lee
openalex +1 more source
SDSS-C4 3028: the Nearest Blue Galaxy Cluster Devoid of an Intracluster Medium
SDSS-C4 3028 is a galaxy cluster at $z=0.061$, notable for its unusually high fraction of star-forming galaxies with 19 star-forming and 11 quiescent spectroscopically-confirmed member galaxies. From Subaru/HSC imaging, we derived a weak lensing mass of $
Shweta Jain +11 more
doaj +1 more source

