Fermi-LAT Observations of γ-Ray Emission toward the Outer Halo of M31. [PDF]
Karwin CM+3 more
europepmc +1 more source
Altered hepatic metabolic landscape and insulin sensitivity in response to pulmonary tuberculosis. [PDF]
Das MK+7 more
europepmc +1 more source
HEXB Drives Raised Paucimannosylation in Colorectal Cancer and Stratifies Patient Risk. [PDF]
Kawahara R+7 more
europepmc +1 more source
lntrinsic morphology and global kinematics of Andromeda satellite galaxies
J.-B. Salomon
openalex +1 more source
Pulsating red giant and supergiant stars in the Local Group dwarf galaxy Andromeda I
Elham Saremi+4 more
doaj +1 more source
Defending the quantum reconstruction program. [PDF]
Berghofer P.
europepmc +1 more source
The remnant of a merger between two dwarf galaxies in Andromeda II [PDF]
Driven by gravity, massive structures like galaxies and clusters of galaxies are believed to grow continuously through hierarchical merging and accretion of smaller systems. Observational evidence of accretion events is provided by the coherent stellar streams crossing the outer haloes of massive galaxies, such as the Milky Way or Andromeda. At similar
Glenn Van De Ven
exaly +2 more sources
Andromeda IX: A New Dwarf Spheroidal Satellite of M31 [PDF]
We report the discovery of a new dwarf spheroidal satellite of M31, Andromeda IX, based on resolved stellar photometry from the Sloan Digital Sky Survey (SDSS). Using both SDSS and public archival data we have estimated its distance and other physical properties, and compared these to the properties of a previously known dwarf spheroidal companion ...
Daniel B Zucker+2 more
exaly +2 more sources
ANDROMEDA XXVIII: A DWARF GALAXY MORE THAN 350 kpc FROM ANDROMEDA [PDF]
We report the discovery of a new dwarf galaxy, Andromeda XXVIII, using data from the recently-released SDSS DR8. The galaxy is a likely satellite of Andromeda, and, at a separation of $365^{+17}_{-1}$ kpc, would be one of the most distant of Andromeda's satellites.
Eric F Bell, Nicolas F Martin
exaly +2 more sources
The Faint Globular Cluster in the Dwarf Galaxy Andromeda I [PDF]
Observations of globular clusters in dwarf galaxies can be used to study a variety of topics, including the structure of dark matter halos and the history of vigorous star formation in low-mass galaxies. We report on the properties of the faint globular cluster (M_V ~ -3.4) in the M31 dwarf galaxy Andromeda I. This object adds to the growing population
Anil C Seth, David J Sand, Jay Strader
exaly +2 more sources