Results 121 to 130 of about 89,941 (303)
A Slowly Pulsating Run‐Away B Star at High Galactic Latitude Ejected From a Spiral Arm
ABSTRACT We report the discovery of the young B6 V run‐away star LAMOST J083323.18 + 430825.4, 2.5 kpc above the Galactic plane. Its atmospheric parameters and chemical composition are determined from LAMOST spectra, indicating normal composition. Effective temperature (Teff$$ {T}_{\mathrm{eff}} $$ = 14,500$$ \mathrm{14,500} $$ K) and gravity (logg ...
Ulrich Heber+3 more
wiley +1 more source
Turbulent heating in galaxy clusters brightest in X-rays [PDF]
published in ...
Aurora Simionescu+13 more
openaire +10 more sources
The Evolution of AGN Activity in Brightest Cluster Galaxies
Abstract We present the results of an analysis of Wide-field Infrared Survey Explorer (WISE) observations of the full 2500 deg2 South Pole Telescope (SPT)-Sunyaev–Zel’dovich cluster sample. We describe a process for identifying active galactic nuclei (AGN) in brightest cluster galaxies (BCGs) based on WISE mid-IR color and redshift ...
Taweewat Somboonpanyakul+81 more
openaire +9 more sources
Extended Radio Emission in the Perhipheral Regions of the Shapley Concentration Core
The Shapley Concentration (SC) is a galaxy supercluster (few tens of degrees) in the Local Universe (<z>∼0.048) which is currently undergoing cluster mergers and group accretion.
Tiziana Venturi+6 more
doaj +1 more source
Intermittent, mild pro‐inflammatory systemic disease contributes to cerebrovascular pathology, however the mechanism of low‐level exposure causing injury remains unclear. Our RNA‐Seq analysis reveals continuous activation of tumour necrosis factor (TNF)‐Nuclear Factor kappa B (NF‐κB) signalling and multiple downstream inflammatory mediators in mouse ...
Megan Ritson+3 more
wiley +1 more source
Volume measurement of microparticles using SEM photogrammetry and 3‐D reconstruction
Abstract In this paper, we introduce a method for volume measurement of microparticles that includes scanning electron microscope photogrammetry with 3‐D model construction. Our results show that our method limits the volume uncertainty to ±10%, which is a significant improvement compared to previous methods (which likely overestimated volume by 100 ...
Y. Zheng+4 more
wiley +1 more source
WITNESSING THE FORMATION OF A BRIGHTEST CLUSTER GALAXY IN A NEARBY X-RAY CLUSTER [PDF]
The central dominant galaxies in galaxy clusters constitute the most massive and luminous galaxies in the universe. Despite this, the formation of these brightest cluster galaxies (BCGs) and the impact of this on the surrounding cluster environment ...
J. Rasmussen+5 more
semanticscholar +1 more source
Models for the magnitude-distribution of brightest cluster galaxies [PDF]
Abstract submitted to AAS.
J. P. Bernstein+2 more
openaire +4 more sources
Do arcs require flat halo cusps?
It was recently claimed that several galaxy clusters containing radial and tangential gravitational arcs and having a measured velocity-dispersion profile for the brightest cluster galaxy had to have central density profiles considerably flatter than ...
Bartelmann+10 more
core +1 more source
Cluster detection from surface-brightness fluctuations in SDSS data [PDF]
Galaxy clusters can be detected as surface brightness enhancements in smoothed optical surveys. This method does not require individual galaxies to be identifiable, and enables clusters to be detected out to surprisingly high redshifts, as recently ...
Aragón-Salamanca+24 more
core +2 more sources