Results 11 to 20 of about 92,409 (330)
INSIGHT INTO THE FORMATION OF THE MILKY WAY THROUGH COLD HALO SUBSTRUCTURE. I. THE ECHOS OF MILKY WAY FORMATION [PDF]
The Astrophysical Journal, 2009 47 pages, 23 figures, and 6 tables in emulaetapj format; accepted for publication in ...
Kevin C. Schlaufman +13 more
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Abundance Gradients and the Formation of the Milky Way [PDF]
The Astrophysical Journal, 2001 In this paper we adopt a chemical evolution model, which is an improved version of the Chiappini, Matteucci and Gratton (1997) model, assuming two main accretion episodes for the formation of the Galaxy. The present model takes into account in more detail than previously the halo density distribution and explores the effects of a threshold density in ...
CHIAPPINI C. +2 more
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Star Formation in the Milky Way: The Infrared View [PDF]
, 2013 12 pages, 9 figures. To apper in "Cosmic-ray induced phenomenology in star-forming environments: Proceedings of the 2nd Session of the Sant Cugat Forum of Astrophysics" (April 16-19, 2012), Olaf Reimer and Diego F. Torres (eds.)
A Heiderman +23 more
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THE FORMATION OF THE MILKY WAY IN THE COSMOLOGICAL CONTEXT [PDF]
, 2001 5 pages, conference proceeding. to appear in "Cosmic Evolution", eds. M. Lemoine and E.
Burkert, Andreas
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The simulation of molecular clouds formation in the Milky Way [PDF]
, 2012 Using 3D hydrodynamic calculations we simulate formation of molecular clouds in the Galaxy. The simulations take into account molecular hydrogen chemical kinetics, cooling and heating processes.
Sergey Khoperskov +3 more
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DISSIPATIONLESS FORMATION AND EVOLUTION OF THE MILKY WAY NUCLEAR STAR CLUSTER [PDF]
, 2012 Abridged: In one widely discussed model for the formation of nuclear star clusters (NSCs), massive globular clusters spiral into the center of a galaxy and merge to form the nucleus. It is now known that at least some NSCs coexist with supermassive black
Fabio Antonini +3 more
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Chemodynamical Analysis of Metal-rich High-eccentricity Stars in the Milky Way's Disk
The Astrophysical Journal, 2023 We present a chemodynamical analysis of 11,562 metal-rich, high-eccentricity halo-like main-sequence stars, which have been referred to as the Splash or Splashed Disk, selected from the Sloan Digital Sky Survey and Large Sky Area Multi-Object Fiber ...
Ayeon Lee +4 more
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Star formation law in the Milky Way [PDF]
Publications of the Astronomical Society of Japan, 2017 Abstract The Schmidt law (SF law) in the Milky Way was investigated using 3D distribution maps of H ii regions and H i and molecular (H2) gases with spatial resolutions of ∼1 kpc in the Galactic plane and a few tens of pc in the vertical direction. H ii regions were shown to be distributed in a star-forming (SF) disk with nearly constant
Sofue, Yoshiaki, Nakanishi, Hiroyuki
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STAR FORMATION RELATIONS IN THE MILKY WAY [PDF]
The Astrophysical Journal, 2016 ABSTRACT The relations between star formation and properties of molecular clouds (MCs) are studied based on a sample of star-forming regions in the Galactic Plane. Sources were selected by having radio recombination lines to provide identification of associated MCs and dense clumps. Radio continuum emission and mid-infrared emission were
Nalin Vutisalchavakul +2 more
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Momento, 2014 At present there is some evidence showing that the satellite galaxies of the Milky Way might be distributed on a disc structure, known as the disc of satellites.
Diana J. Cubillos Jara +1 more
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