Results 31 to 40 of about 92,409 (330)
GTC Follow-up Observations of Very Metal-poor Star Candidates from DESI
The observations from the Dark Energy Spectroscopic Instrument (DESI) will significantly increase the numbers of known extremely metal-poor stars by a factor of ∼10, improving the sample statistics to study the early chemical evolution of the Milky Way ...
Carlos Allende Prieto +50 more
doaj +1 more source
Radial structure and formation of the Milky Way disc [PDF]
Context. The formation of the Galactic disc is an enthusiastically debated issue. Numerous studies and models seek to identify the dominant physical process(es) that shaped its observed properties; for example, satellite accretion, starburst, quenching, gas infall, and stellar radial migration. Aims.
Katz, D. +4 more
openaire +3 more sources
How Does Feedback Affect Milky Way Satellite Formation? [PDF]
Oral Presentation, Proceedings of "A Universe of Dwarf Galaxies" Conference, Lyon ...
Geen, S, Slyz, A, Devriendt, J
openaire +3 more sources
We review observational evidence bearing on the formation of a prototypical large spiral galaxy, the Milky Way. New ground- and space-based studies of globular star clusters and dwarf spheroidal galaxies provide a wealth of information to constrain theories of galaxy formation.
Hesser, J. E. +11 more
openaire +2 more sources
The origin of the Milky Way globular clusters [PDF]
We present a cosmological zoom-in simulation of a Milky Way-like galaxy used to explore the formation and evolution of star clusters. We investigate in particular the origin of the bimodality observed in the colour and metallicity of globular clusters ...
Agertz, Oscar +2 more
core +2 more sources
Star Formation in the Local Milky Way [PDF]
AbstractStudies of molecular clouds and young stars near the sun have provided invaluable insights into the process of star formation. Indeed, much of our physical understanding of this topic has been derived from such studies. Perhaps the two most fundamental problems confronting star formation research today are: 1) determining the origin of stellar ...
openaire +2 more sources
Dense gas and star formation in the outer Milky Way
We present maps and spectra of the HCN(1−0) and HCO+(1−0) lines in the extreme outer Galaxy, at galactocentric radii between 14 and 22 kpc, with the 13.7 m Delingha telescope. The nine molecular clouds were selected from a CO/13CO survey of the outer quadrants.
Braine, J. +7 more
openaire +3 more sources
Simulations of the Milky Way’s Central Molecular Zone – II. Star formation [PDF]
ABSTRACTThe Milky Way’s Central Molecular Zone (CMZ) has emerged in recent years as a unique laboratory for the study of star formation. Here we use the simulations presented in Tress et al. to investigate star formation in the CMZ. These simulations resolve the structure of the interstellar medium at sub-parsec resolution while also including the ...
Mattia C Sormani +7 more
openaire +3 more sources
The origin of physical variations in the star formation law [PDF]
Observations of external galaxies and of local star-forming clouds in the Milky Way have suggested a variety of star formation laws, i.e., simple direct relations between the column density of star formation (Sigma_SFR: the amount of gas forming stars ...
Federrath, Christoph
core +1 more source
The Milky Way is the only galaxy for which we can resolve individual stars at all evolutionary phases, from the Galactic center to the outskirt. The last decade, thanks to the advent of near IR detectors and 8 meter class telescopes, has seen a great ...
Alard +15 more
core +1 more source

