Results 91 to 100 of about 370,839 (289)
Is the Andromeda galaxy approaching our galaxy Milky Way?
Nodoubt that thedarkenergycarrier interactswiththebaryonicmatter. Due tothis interaction someportionsofenergyaretransferringgraduallytoallbaryonicobjectsandtheirsystemswithoutany exceptionatallhierarchical levelsof thebaryonicworld.
H. Harutyunian+3 more
semanticscholar +1 more source
Search for dark matter gamma-ray emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory [PDF]
The Andromeda Galaxy (M31) is a nearby (∼780 kpc) galaxy similar to our own Milky Way. Observational evidence suggests that it resides in a large halo of dark matter (DM), making it a good target for DM searches.
A. Albert+101 more
semanticscholar +1 more source
We present results from wide-field imaging of the resolved stellar populations of the dwarf spheroidal galaxies Cassiopeia III (And XXXII) and Perseus I (And XXXIII), two satellites in the outer stellar halo of the Andromeda galaxy (M31).
Katherine L. Rhode+10 more
doaj +1 more source
THEHERSCHELEXPLOITATION OF LOCAL GALAXY ANDROMEDA (HELGA). II. DUST AND GAS IN ANDROMEDA [PDF]
We present an analysis of the dust and gas in Andromeda, using Herschel images sampling the entire far-infrared peak. We fit a modified-blackbody model to ~4000 quasi-independent pixels with spatial resolution of ~140pc and find that a variable dust-emissivity index (beta) is required to fit the data. We find no significant long-wavelength excess above
Luigi Spinoglio+30 more
openaire +11 more sources
Collision tomography: Physical properties of possible progenitors of the Andromeda stellar stream [PDF]
To unveil a progenitor of the Andromeda Giant Stellar Stream, we investigate the interaction between an accreting satellite galaxy and the Andromeda Galaxy using an $N$-body simulation. A comprehensive parameter study with 247 models is performed by varying size and mass distribution of the progenitor dwarf galaxy.
arxiv +1 more source
A New Giant Stellar Structure in the Outer Halo of M31
The Sloan Digital Sky Survey has revealed an overdensity of luminous red giant stars ~ 3 degrees (40 projected kpc) to the northeast of M31, which we have called Andromeda NE.
Bell, Eric F.+19 more
core +2 more sources
A New Luminous Blue Variable in the Outskirts of the Andromeda Galaxy [PDF]
The hot massive luminous blue variables (LBVs) represent an important evolutionary phase of massive stars. Here, we report the discovery of a new LBV—LAMOST J0037+4016 in the distant outskirt of the Andromeda galaxy.
Yang Huang+10 more
semanticscholar +1 more source
We present spectroscopic chemical abundances of red giant branch stars in Andromeda (M31), using medium-resolution ( R ∼ 6000) spectra obtained via the Spectroscopic and Photometric Landscape of Andromeda’s Stellar Halo survey.
J. Leigh Wojno+8 more
doaj +1 more source
Ellipticities of Globular Clusters in the Andromeda Galaxy [PDF]
A program of investigation of globular clusters' structural parameters in nearby galaxies has been initiated at the Rozhen National Observatory, Bulgaria (Spassova and Staneva 1984). Here we report on the projected ellipticities of 88 bright globular clusters in M 31, obtained on plates taken with the 2 m Ritchey-Chretien telescope at Rozhen (16 m ...
Nedka M. Spassova+2 more
openaire +3 more sources
Scientific photography and astronomy: Technology applied to understanding the universe
In 1925, Edwin Hubble took the first step towards increasing the size of the known universe by several orders of magnitude using the precarious photographic methods available at the time: glass plates and photosensitive emulsions.
Fernando Abalos Vazquez, Javier Ábalos
doaj +1 more source