Results 141 to 150 of about 2,066,093 (377)
Galactic globular clusters consist of two main stellar populations, the pristine (1P) and polluted (2P) stars. The fraction of 1P stars in clusters, F _1P , is a decreasing function of the present-day cluster mass, m _prst . The information about cluster
Geneviève Parmentier
doaj +1 more source
In the context of a project aimed at characterizing the dynamical evolution of old globular clusters in the Large Magellanic Cloud, we have secured deep HST/WFC3 images of the massive cluster NGC 1835.
Camilla Giusti +8 more
doaj +1 more source
The Observational and Theoretical Tidal Radii of Globular Clusters in M87
Globular clusters have linear sizes (tidal radii) which theory tells us are determined by their masses and by the gravitational potential of their host galaxy.
Alison Sills +24 more
core +1 more source
This study investigates gene expression differences between two major pediatric acute lymphoblastic leukemia (ALL) subtypes, B‐cell precursor ALL, and T‐cell ALL, using a data‐driven approach consisting of biostatistics and machine learning methods. Following analysis of a discovery dataset, we find a set of 14 expression markers differentiating the ...
Mona Nourbakhsh +8 more
wiley +1 more source
The SLUGGS Survey: wide field imaging of the globular cluster system of NGC 4278 [PDF]
We use multipointing Hubble Space Telescope Advanced Camera for Surveys and wide field Subaru Suprime-Cam imaging to study the globular cluster system of the L ∗ elliptical galaxy NGC 4278.
C. Usher +6 more
semanticscholar +1 more source
Unraveling LINE‐1 retrotransposition in head and neck squamous cell carcinoma
The novel RetroTest method allows the detection of L1 activation in clinical samples with low DNA input, providing global L1 activity and the identification of the L1 source element. We applied RetroTest to a real‐world cohort of HNSCC patients where we reported an early L1 activation, with more than 60% of T1 patients showing L1 activity.
Jenifer Brea‐Iglesias +12 more
wiley +1 more source
The Extended Baryonic Halo of NGC 3923
Galaxy halos and their globular cluster systems build up over time by the accretion of small satellites. We can learn about this process in detail by observing systems with ongoing accretion events and comparing the data with simulations.
Bryan W. Miller +9 more
doaj +1 more source
RUPRECHT 106: THE FIRST SINGLE POPULATION GLOBULAR CLUSTER? [PDF]
All old Galactic globular clusters (GCs) studied in detail to date host at least two generations of stars, where the second is formed from gas polluted by processed material produced by massive stars of the first.
S. Villanova +4 more
semanticscholar +1 more source
Star-Forming Galaxies at z~2 and the Formation of the Metal-Rich Globular Cluster Population
We examine whether the super star-forming clumps (R~1-3 kpc; M~10^8-10^9.5 Msun) now known to be a key component of star-forming galaxies at z~2 could be the formation sites of the locally observed old globular cluster population.
Armandroff +71 more
core +1 more source
Globular Clusters and Galaxy Formation [PDF]
8 pages, 6 figures, Globular Clusters - Guides to Galaxies ...
openaire +4 more sources

