Results 101 to 110 of about 210,241 (186)
Shell Structure in the Fornax Dwarf Spheroidal Galaxy
We present initial results from a wide-field photometric survey of the Fornax dwarf spheroidal (dSph) galaxy. The focus here is on a small overdensity of stars located approximately 17' (670 pc in projection) from the center of Fornax. Based
Bland-Hawthorn, Joss +5 more
core +1 more source
Feeding and feedback in dwarf galaxies (FeeD)
Feeding and feedback regulated by supermassive black holes play a central role in galaxy growth and evolution, yet these processes remain poorly understood in low-mass galaxies.
Mondal S. +7 more
doaj +1 more source
Dark matter indirect detection from dwarf spheroidal galaxies (dSphs) and galaxy clusters
Maurin, David. (2013). Dark matter indirect detection from dwarf spheroidal galaxies (dSphs) and galaxy clusters.
Maurin, D., Maurin, David
core
We are entering an era in which we will be able to detect and characterize hundreds of dwarf galaxies within the Local Volume. It is already known that a strong dichotomy exists in the gas content and star formation properties of field dwarf galaxies ...
Charlotte R. Christensen +7 more
doaj +1 more source
A spectroscopic binary in the Hercules dwarf spheroidal galaxy
We present the radial velocity curve of a single-lined spectroscopic binary in the faint Hercules dwarf spheroidal (dSph) galaxy, based on 34 individual spectra covering more than 2 yr of observations.
Feltzing, S. +8 more
core +1 more source
Intermediate Mass Ratio Inspirals in Milky Way Galaxies
A consequence of a nonzero occupation fraction of massive black holes (MBHs) in dwarf galaxies is that these MBHs can become residents of larger galaxy halos via hierarchical merging and tidal stripping.
Jillian Bellovary +5 more
doaj +1 more source
Dwarf galaxy mass estimators versus cosmological simulations. [PDF]
González-Samaniego A +7 more
europepmc +1 more source
Towards AMR Simulations of Galaxy Formation [PDF]
Numerical simulations present a fundamental building block of our modern theoretical understanding of the Universe. As such the work in this thesis is primarily concerned with understanding fundamental differences that lie between the different ...
MITCHELL, NIGEL,LEWIS +1 more
core
Chemical Cartography of the Sagittarius Stream with Gaia
The stellar stream connected to the Sagittarius (Sgr) dwarf galaxy is the most massive tidal stream that has been mapped in the Galaxy, and is the dominant contributor to the outer stellar halo of the Milky Way (MW).
Emily C. Cunningham +7 more
doaj +1 more source
GHOSTS I : a new faint very isolated dwarf galaxy at D = 12 ± 2 Mpc.
We report the discovery of a new faint dwarf galaxy, GHOSTS I, using HST/ACS data from one of our GHOSTS (Galaxy Halos, Outer disks, Substructure, Thick disk, and Star clusters) fields.
Streich, David +10 more
core +1 more source

