Results 71 to 80 of about 234,039 (316)

Baryons in Dark Matter Halos [PDF]

open access: yes, 2004
6 ...
Dettmar RJ, Klein U, Salucci, Paolo
openaire   +2 more sources

Inhibition of acyl‐CoA synthetase long‐chain isozymes decreases multiple myeloma cell proliferation and causes mitochondrial dysfunction

open access: yesMolecular Oncology, EarlyView.
Triacsin C inhibition of the acyl‐CoA synthetase long chain (ACSL) family decreases multiple myeloma cell survival, proliferation, mitochondrial respiration, and membrane potential. Made with Biorender.com. Multiple myeloma (MM) is an incurable cancer of plasma cells with a 5‐year survival rate of 59%.
Connor S. Murphy   +12 more
wiley   +1 more source

Constraining the Gravitational Potential from the Projected Morphology of Extragalactic Tidal Streams

open access: yesThe Astrophysical Journal, 2023
The positions and velocities of stellar streams have been used to constrain the mass and shape of the Milky Way's dark matter halo. Several extragalactic streams have already been detected, though it has remained unclear what can be inferred about the ...
Jacob Nibauer   +2 more
doaj   +1 more source

Galaxy Disruption in a Halo of Dark Matter

open access: yesScience, 2003
The relics of disrupted satellite galaxies have been found around the Milky Way and Andromeda, but direct evidence of a satellite galaxy in the early stages of disruption has remained elusive. We have discovered a dwarf satellite galaxy in the process of being torn apart by gravitational tidal forces as it merges with a larger galaxy's dark matter halo.
Forbes, Duncan A.   +4 more
openaire   +5 more sources

Mapping substructures in dark matter haloes [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2005
Abstract We present a detailed study of the real and integrals-of-motion space distributions of a disrupting satellite obtained from a fully self-consistent high-resolution cosmological simulation of a galaxy cluster. The satellite has been re-simulated using various analytical halo potentials, and we find that its debris appears as a ...
Knebe, Alexander   +3 more
openaire   +4 more sources

Targeting PRAME directly or via EZH2 inhibition overcomes retinoid resistance and represents a novel therapy for keratinocyte carcinoma

open access: yesMolecular Oncology, EarlyView.
The study evaluated the function and therapeutic implications of PRAME in basal cell carcinoma (BCC) and squamous cell carcinoma (SCC). The findings demonstrate that PRAME impairs keratinocyte differentiation pathways. Furthermore, PRAME impairs anticancer response to retinoid compounds in BCC and SCC cells.
Brandon Ramchatesingh   +6 more
wiley   +1 more source

Using frequency maps to explore the distribution function of the Milky Way stellar halo

open access: yesEPJ Web of Conferences, 2012
Resolved surveys of the Milky Way's stellar halo can obtain all 6 phase space coordinates of tens of thousands of individual stars, making it possible to compute their 3-dimensional orbits.
Valluri M.
doaj   +1 more source

Halo uncertainties in electron recoil events at direct detection experiments

open access: yesEuropean Physical Journal C: Particles and Fields, 2021
The dark matter direct detection rates are highly correlated with the phase space distribution of dark matter particles in our galactic neighbourhood.
Tarak Nath Maity   +2 more
doaj   +1 more source

On the Possible Asymmetry in Gamma Rays from Andromeda Due to Inverse Compton Scattering of Star Light on Electrons from Dark Matter Annihilation

open access: yesGalaxies, 2023
Dark matter is a popular candidate to a new source of primary-charged particles, especially positrons in cosmic rays, which are proposed to account for observable anomalies.
Konstantin Belotsky, Maxim Solovyov
doaj   +1 more source

Non-universality of halo profiles and implications for dark matter experiments [PDF]

open access: yesMon. Not. Roy. Astron. Soc. 415 (2011) 3177-3188, 2010
We explore the cosmological halo-to-halo scatter of the distribution of mass within dark matter halos utilizing a well-resolved statistical sample of clusters from the cosmological Millennium simulation. We find that at any radius, the spherically-averaged dark matter density of a halo (corresponding to the "smooth-component") and its logarithmic slope
arxiv   +1 more source

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