Results 11 to 20 of about 216,057 (315)
Mapping the Galactic halo with main-sequence and RR Lyrae stars [PDF]
We present an analysis of Galactic halo structure, substructure, and metallicity traced by main-sequence and RR Lyrae stars selected from the SDSS stripe 82 and CFHT Legacy Survey data sets.
Sesar B.
doaj +2 more sources
Galactic Halo Wormhole Solutions in f(T) Gravity
The proposal of galactic halo region is based on the idea that dark halos contain some characteristics needed to support traversable wormhole solutions. We explore wormhole solutions in this region in the framework of generalized teleparallel gravity. We
M. Sharif, Shamaila Rani
doaj +2 more sources
Solutions of the Einstein Equations for a Black Hole Surrounded by a Galactic Halo [PDF]
Various profiles of matter distribution in galactic halos (such as the Navarro–Frenk–White, Burkert, Hernquist, Moore, Taylor–Silk models, and others) are considered here as the source term for the Einstein equations.
R. Konoplya, A. Zhidenko
semanticscholar +1 more source
In this article, we find the possibility of generalized wormhole formation in the galactic halo due to dark matter using observational data within the matter coupling gravity formalism.
G. Mustafa, S. K. Maurya, Saibal Ray
semanticscholar +1 more source
The CHIME/FRB project has detected hundreds of fast radio bursts (FRBs), providing an unparalleled population to statistically probe the foreground media that they illuminate. One such foreground medium is the ionized halo of the Milky Way (MW).
Amanda M. Cook +27 more
doaj +1 more source
Galactic Wormhole under Lovelock Gravity
We explore wormhole geometry in spiral galaxies under the third order Lovelock gravity. Using the cubic spline interpolation technique, we find the rotational velocity of test particles in the halo region of our spiral galaxy from observed values of ...
Koushik Chakraborty +4 more
doaj +1 more source
Detection of the LMC-induced sloshing of the Galactic halo [PDF]
A wealth of recent studies have shown that the LMC is likely massive, with a halo mass >1011 M⊙. One consequence of having such a nearby and massive neighbour is that the inner Milky Way is expected to be accelerated with respect to our Galaxy’s ...
D. Erkal +10 more
semanticscholar +1 more source
Probing the Galactic Halo with RR Lyrae Stars. I. The Catalog [PDF]
We present a catalog of 5290 RR Lyrae stars (RRLs) with metallicities estimated from spectra of the LAMOST Experiment for Galactic Understanding and Exploration (LEGUE) and the Sloan Extension for Galactic Understanding and Exploration (SEGUE) surveys ...
G.-C. Liu +12 more
semanticscholar +1 more source
Pressure at the ISM-halo interface: A reheating frequency dependence [PDF]
The dependence of the thermal pressure of hot galactic halos on a model parameter describing the frequency of major reheating episodes during galactic history is investigated.
Ćirković M.M.
doaj +1 more source
Low-frequency Faraday rotation measures towards pulsars using LOFAR: probing the 3D Galactic halo magnetic field [PDF]
We determined Faraday rotation measures (RMs) towards 137 pulsars in the northern sky, using Low-Frequency Array (LOFAR) observations at 110–190 MHz. This low-frequency RM catalogue, the largest to date, improves the precision of existing RM measurements
C. Sobey +46 more
semanticscholar +1 more source

