Supernova Remnants in the Local Group I: A model for the radio luminosity function and visibility times of supernova remnants [PDF]
, 2016 Supernova remnants (SNRs) in Local Group galaxies offer unique insights into the origin of different types of supernovae. In order to take full advantage of these insights, one must understand the intrinsic and environmental diversity of SNRs in the ...
S. Sarbadhicary +4 more
semanticscholar +1 more source
BMC Public Health, 2018 Background The main objective of this study was to test some of the draft sexual health indicators developed by the World Health Organization as part of a comprehensive indicator framework to monitor progress in universal access to reproductive health ...
Cinta Folch +5 more
doaj +1 more source
Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies. [PDF]
, 2016 We study galaxy formation in sterile neutrino dark matter models that differ significantly from both cold and from `warm thermal relic' models. We use the EAGLE code to carry out hydrodynamic simulations of the evolution of pairs of galaxies chosen to ...
M. Lovell +12 more
semanticscholar +1 more source
Morphological transformation of dwarf galaxies in the Local Group [PDF]
, 2015 In the Local Group there are three main types of dwarf galaxies: Dwarf Irregulars, Dwarf Spheroidals, and Dwarf Ellipticals. Intermediate/transitional types are present as well.
Carraro, Giovanni
core +1 more source
Resilience strategies of West African pastoralists in response to scarce forage resources
Pastoralism, 2021 Finding sufficient natural fodder resources to feed livestock has become a challenge for herders in the Sahel zone of Burkina Faso. Despite the existence of pastoral reserves, the issue of fodder shortage remains unsolved.
Karim Ouédraogo +4 more
doaj +1 more source
On the origins of enigmatic stellar populations in Local Group galactic nuclei [PDF]
, 2016 We consider the origins of enigmatic stellar populations in four Local Group galactic nuclei, specifically the Milky Way, M31, M32 and M33. These are centrally concentrated blue stars, found in three out of the four nuclear star clusters (NSCs ...
N. Leigh +4 more
semanticscholar +1 more source
Renormalization group aspects of the local composite operator method [PDF]
, 2006 We review the current status of the application of the local composite operator technique to the condensation of dimension two operators in quantum chromodynamics (QCD).
Browne, R. E. +7 more
core +3 more sources
Line-of-Sight Mass Estimator and the Masses of the Milky Way and Andromeda Galaxy
UniverseThe total mass of a galaxy group, such as the Milky Way (MW) and the Andromeda Galaxy (M 31), is typically determined from the kinematics of satellites within their virial zones. Bahcall and Tremaine (1981) proposed the v2r estimator as an alternative to
Danila Makarov +3 more
doaj +1 more source
The local group: The ultimate deep field [PDF]
, 2016 Author(s): Boylan-Kolchin, M; Weisz, DR; Bullock, JS; Cooper, MC | Abstract: © 2016 The Authors. Near-field cosmology - using detailed observations of the Local Group and its environs to study wide-ranging questions in galaxy formation and dark matter ...
M. Boylan-Kolchin +3 more
semanticscholar +1 more source
Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations [PDF]
, 2012 We use the recently proposed scale-free mass estimators to determine the masses of the Milky Way (MW) and Andromeda (M31) galaxy in a dark matter only Constrained Local UniversE Simulation (CLUES).
Alexander Knebe +57 more
core +2 more sources