Results 91 to 100 of about 887 (163)
The Emergence of a Brightest Cluster Galaxy in a Protocluster Core at z = 2.24
We report the detection of a pair of massive quiescent galaxies likely in the process of merging at the center of the spectroscopically confirmed, extremely massive protocluster BOSS1244 at z = 2.24 ± 0.02.
Dong Dong Shi+6 more
doaj +1 more source
White Dwarf Stars in the Big Data Era
ABSTRACT White dwarf stars are the most common endpoint of stellar evolution. Therefore, these old, numerous and compact objects provide valuable information on the late stages of stellar evolution, the physics of dense plasma and the structure and evolution of our Galaxy.
Maria Camisassa
wiley +1 more source
ABSTRACT Observations show that the x‐ray emission of the accreting weakly magnetized neutron stars (WMNSs) is polarized. In this article, we summarize the analytical models for the polarized emission of various components of the WMNSs. We introduce a missing theoretical model, where we assume the emission comes from the spreading layer, the extension ...
Anna Bobrikova, Sofia V. Forsblom
wiley +1 more source
ABSTRACT Objectives Hirsutism is a widespread condition affecting 5%–15% of females. Laser treatment of hirsutism has the best long‐term effect. Patients with nonpigmented or nonterminal hairs are not eligible for laser treatment, and the current patient journey needed to establish eligibility for laser hair removal is problematic in many health‐care ...
Kenneth Thomsen+11 more
wiley +1 more source
Molecular techniques in haematopathology: what and how?
Schematic representation of various molecular alterations relevant to lymphoid and myeloid neoplasms and the different techniques that can be used for detection. Here we review the ‘what and how’ of molecular techniques used in the context of haematopathological diagnostics of both lymphoid and myeloid neoplasms.
Gaurav Chatterjee+4 more
wiley +1 more source
Measuring the optical depth profile of galaxy clusters by kinetic Sunyaev-Zel\'dovic effect
baryonic matter distribution in the large-scale structures is one of the main questions in cosmology. This distribution can provide valuable information regarding the processes of galaxy formation and evolution.
Sh Baghram
doaj
XRISM Reveals Low Nonthermal Pressure in the Core of the Hot, Relaxed Galaxy Cluster A2029
We present XRISM Resolve observations of the core of the hot, relaxed galaxy cluster Abell 2029 (A2029). We find that the line-of-sight bulk velocity of the intracluster medium (ICM) within the central 180 kpc is at rest with respect to the brightest ...
XRISM Collaboration+138 more
doaj +1 more source
Correlations in Relaxed Clusters of Galaxies
The correlations among different quantities in galaxy clusters, observed by Newman et al. (2013a,b), are investigated. We find an anti-correlation among the slope α, the effective radius, Re, and a correlation among the core radius rcore and Re. Moreover,
Babyk Iu., Del Popolo A.
doaj +1 more source
Weak-lensing Characterization of the Dark Matter in 29 Merging Clusters that Exhibit Radio Relics
We present a multiwavelength analysis of 29 merging galaxy clusters that exhibit radio relics. For each merging system, we perform a weak-lensing analysis on Subaru optical imaging.
Kyle Finner+7 more
doaj +1 more source
We set the stage for reassessing how star formation, emission-line nebulae, and active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs) depend on the thermodynamics of the intracluster medium (ICM).
Arsen Levitskiy+4 more
doaj +1 more source