Results 111 to 120 of about 92,502 (190)
Bulgeless Evolution And the Rise of Discs (BEARD)
We study the formation and evolution of bulgeless galaxies within the Milky Way-Andromeda analogue sample of the TNG50 simulation. Through kinematic decomposition with MORDOR, we identified bulgeless galaxies with a bulge-to-disc mass ratio of B/D ≤ 0.08,
Rosas-Guevara Yetli +22 more
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This thesis work has focused on the Galactic disk kinematics to put some constraints on the scenarios of the thin and thick disk formation. It takes part of the RAVE project which has the goal to spectrocpically measure the radial velocities and the stellar parameters of one million stars in the South celestial hemisphere.
openaire +1 more source
Galaxias Enanas del Grupo Local
The satellite galaxies of the Milky Way are very important both for the studies of the formation and evolution of galaxies and for the research on the dark matter problem. In the present review paper some structural properties of the Local Group, as well
A Casallas Lagos +2 more
doaj
We measure the dependence of planet frequency on host star mass, M _L , and distance from the Galactic center, R _L , using a sample of planets discovered by gravitational microlensing.
Kansuke Nunota +8 more
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Bar formation in the Milky Way type galaxies
8 pages, 5 ...
Polyachenko, E. V. +2 more
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Rising from the Ashes. II. The Bar-driven Abundance Bimodality of the Milky Way
The Milky Way hosts at least two modes in its present-day distribution of Fe and α -elements. The exact cause of this bimodality is disputed, but one class of explanations involves the merger between the Milky Way and a relatively massive satellite (Gaia-
Angus Beane +5 more
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The accretion history of the Milky Way
Dwarf spheroidal galaxies are known to be dominated by old stellar populations. This has led to the assumption that their gas-rich progenitors lost their gas during their infall in the Milky Way (MW) halo at distant look-back times. Here, we report a discovery of a tiny but robustly detected population of possibly young (∼1 Gyr old) and intermediate ...
Yanbin Yang +5 more
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Formation of Galactic Disks. I. Why Did the Milky Way’s Disk Form Unusually Early?
Recent results from spectroscopic and astrometric surveys of nearby stars suggest that the stellar disk of our Milky Way (MW) was formed quite early, within the first few billion years of its evolution.
Vadim A. Semenov +4 more
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Simulations of the formation of a Milky Way like galaxy [PDF]
Die numerische Modellierung der Entstehung einer Milchstraßen ähnlichen Scheibengalaxien ist selbst heute, trotz des Einsatzes modernster Simulationstechniken und leistungsfähiger Großrechner, immer noch nicht zufriedenstellend möglich. Ziel dieser Arbeit ist es, verschiedene Modelle für unterschiedliche Aspekte thermischen sowie kinetischen Feedbacks ...
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Non-Laplacian air-gap electrostatics for high-field oil-water nanoemulsion separation. [PDF]
Panat S +5 more
europepmc +1 more source

