Results 161 to 170 of about 170,345 (283)

A Census of Dwarf Galaxy Satellites around LMC-mass Galaxy NGC 2403

open access: yesThe Astrophysical Journal
We present the first comprehensive census of the satellite population around a Large Magellanic Cloud stellar-mass galaxy, as part of the Magellanic Analog Dwarf Companions and Stellar Halos (MADCASH) survey. We have surveyed NGC 2403 ( D = 3.0 Mpc) with
Jeffrey L. Carlin   +13 more
doaj   +1 more source

Astrophysical site(s) of r-process elements in galactic chemodynamical evolution model

open access: yesEPJ Web of Conferences, 2016
Astrophysical site(s) of rapid neutron-capture process (r-process) is (are) not identified yet. Although core-collapse supernovae have been regarded as one of the possible candidates of the astrophysical site of r-process, nucleosynthesis studies suggest
Hirai Yutaka   +5 more
doaj   +1 more source

LOOKING FOR POSSIBLE DARK MATTER FREE PROGENITORS OF THE CARINA DWARF SPHEROIDAL GALAXY USING N-BODY SIMULATIONS

open access: yesMomento, 2018
We present a study of the evolution of several different dark matter free possible progenitors of the Carina dSph galaxy, one of the satellites of the Milky Way, using Newtonian numerical N-body simulations.
Diego F Castellanos   +1 more
doaj   +1 more source

Overview of the LAMOST survey in the first decade. [PDF]

open access: yesInnovation (Camb), 2022
Yan H   +26 more
europepmc   +1 more source

Dark Matter Searches with the Fermi-LAT in the Direction of Dwarf Spheroidals [PDF]

open access: yesarXiv, 2015
The dwarf spheroidal satellite galaxies of the Milky Way are some of the most dark-matter-dominated objects known. Due to their proximity, high dark matter content, and lack of astrophysical backgrounds, dwarf spheroidal galaxies are widely considered to be among the most promising targets for the indirect detection of dark matter via gamma rays.
arxiv  

The 3.5 keV line from stringy axions

open access: yesJournal of High Energy Physics, 2017
An interesting result in particle astrophysics is the recent detection of an unexplained 3.5 keV line from galaxy clusters. A promising model, which can explain the morphology of the signal and its non-observation in dwarf spheroidal galaxies, involves a
Michele Cicoli   +3 more
doaj   +1 more source

The Kinematics of Dwarf Spheroidal Galaxies

open access: yes, 1997
I review observational data on the kinematic properties of dwarf spheroidal galaxies in the halo of the Milky Way and beyond. The present data confirm previous claims that these galaxies have unusually large central velocity dispersions. `Simple' sources of bias such as binary stars, internal atmospheric motions, measurement errors, and small sample ...
openaire   +2 more sources

Dark matter interpretation of the Fermi-LAT observations toward the outer halo of M31. [PDF]

open access: yesPhys Rev D, 2021
Karwin CM   +5 more
europepmc   +1 more source

Home - About - Disclaimer - Privacy