Results 111 to 120 of about 7,707 (224)
Kinematics and Metallicity of the Dwarf Spheroidal Galaxy Andromeda XVIII
Andromeda XVIII is an isolated dwarf galaxy 579 kpc away from the nearest large galaxy, M31. It is a candidate “backsplash galaxy” that might have been affected by a close passage to M31.
Kateryna A. Kvasova +2 more
doaj +1 more source
AstroSat UVIT Survey of M31: New Compact Source Catalog
An ultraviolet survey of M31 was carried out during 2017–2023 with the UltraViolet Imaging Telescope (UVIT) instrument on board the AstroSat Observatory. Here we present far- and near-ultraviolet (FUV and NUV) observations from the M31 UVIT survey, which
Denis Leahy +3 more
doaj +1 more source
Involucramiento de producto y lealtad de marca para productos de consumo masivo en Bogotá D.C.☆
Mediante este artículo, se busca validar algunas hipótesis referentes a la relación entre involucramiento de pro- ducto y lealtad de marca para productos de consumo masivo en Bogotá (Colombia).
Pedro Julián Ramírez Angulo +1 more
doaj +1 more source
Galactic Centre and M31 EXCESS
Excesses with respect to models of the Galactic diffuse emission in gamma-ray flux have been found around a few GeV at the position of the Galactic Centre (GC) and M31.
FERMI-LAT Collaboration +1 more
core +1 more source
Andromeda XVII:A new low-luminosity satellite of M31 [PDF]
We report the discovery of a new dwarf spheroidal galaxy near M31 on the basis of INT/WFC imaging. The system, Andromeda XVII (And XVII), is located at a projected radius of ≈44 kpc from M31, has a line-of-sight distance of 794 ± 40 kpc measured using ...
Ferguson, A. M.N. +6 more
core +1 more source
La relación gas-polvo en M31 [PDF]
Se estudió la relación gas-polvo en M31. La relación deducida es sustancialmente más baja que la obtenida por van den Bergh (1975), cuyo valor resultó idéntico al que se observa en nuestra Galaxia (Knapp & Kerr, 1974).
Gergely, T.E., Bajaja, Esteban
core
The Panchromatic Hubble Andromeda Southern Treasury (PHAST) is a large 195-orbit Hubble Space Telescope program imaging ∼0.45 deg ^2 of the southern half of M31's star-forming disk at optical and near-ultraviolet (NUV) wavelengths.
Zhuo Chen +27 more
doaj +1 more source
Non-thermal emission in M31 and M33 [PDF]
Context. Spiral galaxies M31 and M33 are among the γ-ray sources detected by the Fermi Large Area Telescope (LAT). Aims. We aim to model the broadband non-thermal emission of the central region of M31 (a LAT point source) and of the disk of M33 (a LAT ...
Massimo Persic +5 more
core +1 more source
Encounters between M33 and Present-day M31 Satellites Hint at a Previous Group Accretion
This work investigates whether two known Andromeda (M31) satellites, Pisces (LGS 3) and Andromeda XVI (And XVI), have interacted with M33, M31’s most massive satellite.
Ekta Patel +4 more
doaj +1 more source
Our neighboring galaxy M31 has been recently surveyed at the far- and near-ultraviolet (FUV and NUV) with the UVIT telescope on AstroSat, which provides unprecedented sensitivity to young stellar populations.
Denis A. Leahy +2 more
doaj +1 more source

