Results 21 to 30 of about 155,710 (341)

Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2023
Chemical abundances are an essential tool in untangling the Milky Way’s enrichment history. However, the evolution of the interstellar medium abundance gradient with cosmic time is lost as a result of radial mixing processes.
B. Ratcliffe   +14 more
semanticscholar   +1 more source

Chemo-dynamical Evolution of Simulated Satellites for a Milky Way–like Galaxy

open access: goldThe Astrophysical Journal
The chemical abundances of Milky Way’s (MW's) satellites reflect their star formation histories (SFHs), yet, due to the difficulty of determining the ages of old stars, the SFHs of most satellites are poorly measured.
Yutaka Hirai   +7 more
doaj   +2 more sources

Evolution of the local spiral structure of the Milky Way revealed by open clusters [PDF]

open access: yesAstronomy & Astrophysics, 2021
The structure and evolution of the spiral arms of our Milky Way are basic but long-standing questions in astronomy. In particular, the lifetime of spiral arms is still a puzzle and has not been well constrained from observations.
C. Hao   +8 more
semanticscholar   +1 more source

Warm dark matter constraints using Milky Way satellite observations and subhalo evolution modeling [PDF]

open access: yesPhysical Review D, 2021
Warm dark matter (WDM) can potentially explain small-scale observations that currently challenge the cold dark matter (CDM) model, as warm particles suppress structure formation due to free-streaming effects.
A. Dekker   +3 more
semanticscholar   +1 more source

The Milky Way as a Key to Structural Evolution in Galaxies

open access: green, 2001
This is a pre-published version which is collected from arXiv link.
Martin D. Weinberg
openalex   +4 more sources

The effects of different Type Ia SN yields on Milky Way chemical evolution [PDF]

open access: yes, 2021
We study the effect of different Type Ia SN nucleosynthesis prescriptions on the Milky Way chemical evolution. To this aim, we run detailed one-infall and two-infall chemical evolution models, adopting a large compilation of yield sets corresponding to ...
M. Palla
semanticscholar   +1 more source

Simulating Atomic Dark Matter in Milky Way Analogs [PDF]

open access: yesAstrophysical Journal Letters, 2023
Dark sector theories naturally lead to multicomponent scenarios for dark matter where a subcomponent can dissipate energy through self-interactions, allowing it to efficiently cool inside galaxies.
Sandip Roy   +5 more
semanticscholar   +1 more source

Connecting the young pulsars in Milky Way globular clusters with white dwarf mergers and the M81 fast radio burst [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2023
The detections of four apparently young radio pulsars in the Milky Way globular clusters are difficult to reconcile with standard neutron star formation scenarios associated with massive star evolution. Here, we discuss formation of these young pulsars
K. Kremer, J. Fuller, A. Piro, S. Ransom
semanticscholar   +1 more source

A Tale of Two Disks: Mapping the Milky Way with the Final Data Release of APOGEE [PDF]

open access: yesAstrophysical Journal, 2023
We present new maps of the Milky Way disk showing the distribution of metallicity ([Fe/H]), α-element abundances ([Mg/Fe]), and stellar age, using a sample of 66,496 red giant stars from the final data release (DR17) of the Apache Point Observatory ...
J. Imig   +26 more
semanticscholar   +1 more source

The Metal-weak Milky Way Stellar Disk Hidden in the Gaia–Sausage–Enceladus Debris: The APOGEE DR17 View

open access: yesThe Astrophysical Journal, 2023
We have for the first time identified the early stellar disk in the Milky Way by using a combination of elemental abundances and kinematics. Using data from APOGEE DR17 and Gaia we select stars in the Mg–Mn–Al–Fe plane with elemental abundances ...
Sofia Feltzing, Diane Feuillet
doaj   +1 more source

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