Results 101 to 110 of about 34,781 (306)
The metallicity distribution function (MDF) and internal chemical variations of a galaxy are fundamental to understand its formation and assembly history.
F. O. Barbosa +29 more
doaj +1 more source
On Dwarf Galaxies as the Source of Intracluster Gas [PDF]
Recent observational evidence for steep dwarf galaxy luminosity functions in several rich clusters has led to speculation that their precursors may be the source of the majority of gas and metals inferred from intracluster medium (ICM) x-ray observations.
Arimoto N. +28 more
core +3 more sources
Space Motions of the Dwarf Spheroidal Galaxies Draco and Sculptor Based on HST Proper Motions with a ∼10 yr Time Baseline [PDF]
We present new proper motion (PM) measurements of the dwarf spheroidal galaxies (dSphs) Draco and Sculptor using multiepoch images obtained with the Hubble Space Telescope ACS/WFC.
S. Sohn +8 more
semanticscholar +1 more source
Dwarf Spheroidal Galaxies in the M101 Group and Behind it [PDF]
published in Astrophysics, v.62, p.293 ...
Karachentsev, I. D., Makarova, L. N.
openaire +2 more sources
Abstract MALDI mass spectrometry imaging (MALDI imaging) uniquely advances cancer research, by measuring spatial distribution of endogenous and exogenous molecules directly from tissue sections. These molecular maps provide valuable insights into basic and translational cancer research, including tumor biology, tumor microenvironment, biomarker ...
Maren Nicole Stillger +4 more
wiley +1 more source
Are Nuclear Star Clusters the Precursors of Massive Black Holes?
We present new upper limits for black hole masses in extremely late type spiral galaxies. We confirm that this class of galaxies has black holes with masses less than 106M⊙, if any. We also derive new upper limits for nuclear star cluster masses in massive galaxies with previously determined black hole masses.
Nadine Neumayer +2 more
wiley +1 more source
Radio-Frequency Searches for Dark Matter in Dwarf Galaxies
Dwarf spheroidal galaxies have long been discussed as optimal targets for indirect dark matter searches. However, the majority of such studies have been conducted with gamma-ray instruments.
Geoff Beck
doaj +1 more source
Phase-space mass bound for fermionic dark matter from dwarf spheroidal galaxies [PDF]
We reconsider the lower bound on the mass of a fermionic dark matter (DM) candidate resulting from the existence of known small Dwarf Spheroidal galaxies, in the hypothesis that their DM halo is constituted by degenerate fermions, with phase-space ...
Chiara Di Paolo, F. Nesti, F. Villante
semanticscholar +1 more source
Updated Bounds on Axion‐Like Particle Dark Matter with the Optical MUSE‐Faint Survey
This study presents bounds on the axion‐like particle (ALP) to two‐photon coupling in the mass range $2.65‐5.27$ eV. The signal from ALP decay are sought in the Multi Unit Spectroscopic Explorer (MUSE) observations of five dwarf spheroidal galaxies, under the assumption that ALPs make up the whole dark matter.
Elisa Todarello
wiley +1 more source
Pulsar‐Driven Jets in Supernovae, Gamma‐Ray Bursts, and the Universe
The bipolarity of Supernova 1987A can be understood through its very early light curve from the CTIO 0.4 m telescope and IUE FES and following speckle observations of the “Mystery Spot”. These indicate a beam/jet of light/particles, with initial collimation factors >104 and velocities >0.95 c, involving up to 10−5 M⊙ interacting with circumstellar ...
John Middleditch +1 more
wiley +1 more source

