Results 111 to 120 of about 12,786 (266)
Little Bear’s pulsating stars: Variable star census of UMi dSph Galaxy
Recent observations and a photometric search for variable stars in the Ursa Minor dwarf spheroidal galaxy (UMi dSph) are presented. Our observations were taken at Apache Point Observatory in 2014 and 2016 using the 0.5m ARCSAT telescope and the West ...
Kinemuchi K. +4 more
doaj +1 more source
[Abridged] Several large scale photometric and spectroscopic surveys are being undertaken to provide a more detailed picture of the Milky Way. Given the necessity of generalisation in the determination of, e.g., stellar parameters when tens and hundred ...
A. S. Árnadóttir +103 more
core +1 more source
Elemental Abundances in And XIX from Coadded Spectra
With a luminosity similar to that of Milky Way dwarf spheroidal systems like Sextans, but a spatial extent similar to that of ultra-diffuse galaxies, Andromeda (And) XIX is an unusual satellite of M31. To investigate the origin of this galaxy, we measure
L. R. Cullinane +8 more
doaj +1 more source
Constraining branon dark matter from observations of the dwarf spheroidal galaxies with the MAGIC telescopes [PDF]
Tjark Miener +4 more
openalex +1 more source
Modeling wave dark matter in dwarf spheroidal galaxies
22 pages, 10 figures, 3 ...
Bray, Hubert L., Parry, Alan R.
openaire +2 more sources
We present our photometric method, which combines Subaru/Hyper Suprime-Cam N B 515, g -band, and i- band filters to distinguish giant stars in Local Group galaxies from Milky Way dwarf contamination.
Keyi Ding +8 more
doaj +1 more source
Implications of elemental abundances in dwarf spheroidal galaxies [PDF]
Unusual elemental abundance patterns observed for stars belonging to nearby dwarf spheroidal (dSph) galaxies are discussed. Analysis of the [alpha/H] vs. [Fe/H] diagrams where alpha represents Mg or average of alpha-elements reveals that Fe from Type Ia supernovae (SNe Ia) does not contribute to the stellar abundances in the dSph galaxies where the ...
openaire +2 more sources
Chemical Properties of Star-Forming Emission Line Galaxies at z=0.1 - 0.5
We measure oxygen and nitrogen abundances for 14 star-forming emission line galaxies (ELGs) at 0 ...
Bender R. +22 more
core +3 more sources
Why Are There Dwarf Spheroidal Galaxies?
4 ApJ pages, submitted to ApJ ...
openaire +2 more sources
Dark Matter And The Habitability of Planets
In many models, dark matter particles can elastically scatter with nuclei in planets, causing those particles to become gravitationally bound. While the energy expected to be released through the subsequent annihilations of dark matter particles in the ...
Hooper, Dan, Steffen, Jason H.
core +1 more source

