Results 71 to 80 of about 7,749 (214)
Chemical Evolution of M31 [PDF]
We review chemical evolution models developed for M31 as well as the abundance determinations available for this galaxy. Then we present a recent chemical evolution model for M31 including radial gas flows and galactic fountains along the disk, as well as a model for the bulge.
Matteucci, F., Spitoni, E.
openaire +2 more sources
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31? [PDF]
Isabel Santos-Santos +2 more
openalex +1 more source
Extinction Distributions in Nearby Star-resolved Galaxies. I. M31
An extinction distribution of the Andromeda galaxy (M31) is constructed with member stars as tracers by fitting multiband photometric data from UKIRT/WFCAM, Panoramic Survey Telescope and Rapid Response System 1, and Gaia DR3.
Yuxi Wang +3 more
doaj +1 more source
Introduction: The Multi-Channel Imager (MCI), one of the back-end modules of the future China Space Station Telescope (CSST), is designed for high-precision spacebased astronomical observations.
Wenfeng Fang +18 more
doaj +1 more source
Deep Andromeda JCMT SCUBA-2 Observations. The Submillimeter Maps and Giant Molecular Clouds
We have carried out unprecedentedly deep, nearly confusion-limited JCMT SCUBA-2 mapping observations on the nearest spiral galaxy, M31 (Andromeda). The 850 μ m image with a ∼50 pc resolution yields a comprehensive catalog of 383 giant molecular clouds ...
Sihan Jiao +25 more
doaj +1 more source
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
We calculate the broad-band spectrum expected of a 10 exp 7 solar mass black hole accreting from an ambient galactic wind in the nucleus of M31, and we discuss several testable predictions of this model: (1) when resolved, this source will probably be elongated, perhaps in the direction of the semistellar nucleus BD +40 148 deg; (2) its radio spectral ...
openaire +1 more source
Tidal Streams and Low Mass Companions of M31 [PDF]
Róbert Braun, David A. Thilker
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Interstellar Polarization in M31
13 pages, 2 figures, AJ in press (June)
Clayton, Geoffrey C. +5 more
openaire +3 more sources
Resolved Stellar Populations of Super-Metal-Rich Star Clusters in the\n Bulge of M31 [PDF]
P. Jablonka +5 more
openalex +1 more source

