Results 121 to 130 of about 85,801 (378)
A Population of Massive Globular Clusters in NGC 5128
, 2004 We present velocity dispersion measurements of 14 globular clusters in NGC 5128 (Centarus A) obtained with the MIKE echelle spectrograph on the 6.5m Magellan Clay telescope.
Battistini P. +8 more
core +1 more source
A search for variable stars in the globular cluster M3 [PDF]
Monthly Notices of the Royal Astronomical Society, 1998 We describe here results of a photometric time-sequence survey of the globular cluster M3 (NGC 5272), in a search for contact and detached eclipsing binary stars. We have discovered only one likely eclipsing binary and one SX Phe type star in spite of monitoring 4077 stars with $V<20.0$ and observing 25 blue stragglers.
Christine M. Clement +3 more
openaire +4 more sources
Molecular Oncology, EarlyView.This study used longitudinal transcriptomics and gene‐pattern classification to uncover patient‐specific mechanisms of chemotherapy resistance in breast cancer. Findings reveal preexisting drug‐tolerant states in primary tumors and diverse gene rewiring patterns across patients, converging on a few dysregulated functional modules. Despite receiving the
Maya Dadiani +14 more
wiley +1 more source
A universal route for the formation of massive star clusters in giant molecular clouds [PDF]
Nature Astronomy, 2018 Young massive clusters (M ≥ 104Mʘ) are proposed modern-day analogues of the globular clusters that were products of extreme star formation in the early Universe1–4.
Corey S. Howard, R. Pudritz, W. Harris
semanticscholar +1 more source
Variable stars in the globular cluster M 92 [PDF]
Astronomy & Astrophysics, 2001 AbstractResults of a search for variable stars in the central region of the Oosterhoff II type globular cluster M92 are presented.
openaire +4 more sources
A CH star in the globular cluster NGC 6426 [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2012 Abstract We report on the serendipitous discovery of a carbon star near the centre of the low-metallicity globular cluster NGC 6426. We determined its membership and chemical properties using medium-resolution spectra. The radial velocity of −159 km s−1 makes it a member of the cluster.
Sharina, M. +4 more
openaire +5 more sources
Molecular Oncology, EarlyView.B‐cell chronic lymphocytic leukemia (B‐CLL) and monoclonal B‐cell lymphocytosis (MBL) show altered proteomes and phosphoproteomes, analyzed using mass spectrometry, protein microarrays, and western blotting. Identifying 2970 proteins and 316 phosphoproteins, including 55 novel phosphopeptides, we reveal BCR and NF‐kβ/STAT3 signaling in disease ...
Paula Díez +17 more
wiley +1 more source
On the Origin of Neutron Stars in Globular Clusters [PDF]
Symposium - International Astronomical Union, 1987 The formation of neutron stars in globular clusters is discussed in light of a number of recent results and, in particular, studies of the origin and evolution of the high luminosity x-ray binaries found in globular clusters. We argue that the neutron stars most probably arise from the accretion-induced collapse of white dwarfs in compact binary ...
openaire +2 more sources
Molecular Oncology, EarlyView.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
Utilizing Voronoi Tessellations to Determine Radial Density Profiles
The Astronomical JournalWe have developed a novel method of determining 2D radial density profiles for astronomical systems of discrete objects using Voronoi tessellations. This Voronoi-based method was tested against the standard annulus-based method on five simulated systems ...
Veronika Dornan, William E. Harris
doaj +1 more source