Connecting the young pulsars in Milky Way globular clusters with white dwarf mergers and the M81 fast radio burst [PDF]
Monthly 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
Evolution of lithium in the Milky Way halo, discs, and bulge [PDF]
Monthly notices of the Royal Astronomical Society, 2019 In this work, we study the Galactic evolution of lithium by means of chemical evolution models in the light of the most recent spectroscopic data from Galactic stellar surveys.
V. Grisoni +3 more
semanticscholar +1 more source
The influence of nova nucleosynthesis on the chemical evolution of the Galaxy [PDF]
, 2000 We adopt up-to-date yields of 7Li, 13C, 15N from classical novae and use a well tested model for the chemical evolution of the Milky Way in order to predict the temporal evolution of these elemental species in the solar neighborhood.
A Renzini +20 more
core +2 more sources
Revisiting long-standing puzzles of the Milky Way: the Sun and its vicinity as typical outer disk chemical evolution [PDF]
Astronomy & Astrophysics, 2019 We present a scenario of the chemical enrichment of the solar neighborhood that solves the G-dwarf problem by taking into account constraints on a larger scale.
M. Haywood +4 more
semanticscholar +1 more source
The formation and early evolution of the Milky Way [PDF]
Symposium - International Astronomical Union, 1985 In broad outline, the traditional picture for the formation of the Milky Way can be summarized as follows. The proto-galaxy consisted of a slowly rotating cloud of metal-free gas that cooled by bremsstrahlung and recombination radiation. As the internal pressure of the gas decreased, it collapsed in stages with smaller dimensions, faster rotation ...
openaire +1 more source
Chemo-spectrophotometric evolution of spiral galaxies: I. The model and the Milky Way [PDF]
, 1999 The chemical and spectro-photometric evolution of spiral galaxies is investigated with detailed models, making use of up-to-date ingredients (like metallicity dependent stellar properties) and a prescription for the star formation rate (SFR) justified ...
Allard +122 more
core +4 more sources
Stellar migrations and metal flows – Chemical evolution of the thin disc of a simulated Milky Way analogous galaxy [PDF]
, 2020 This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society, Volume 496, Issue 1, July 2020, Pages 80–94 ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
F. Vincenzo, C. Kobayashi
semanticscholar +1 more source
The Tilt of the Velocity Ellipsoid of Different Galactic Disk Populations
The Astrophysical Journal, 2023 The tilt of the velocity ellipsoid is a helpful tracer of the gravitational potential of the Milky Way. In this paper, we use nearly 140,000 red clump (RC) stars selected from LAMOST and Gaia to make a detailed analysis of the tilt of the velocity ...
Weixiang Sun, Han Shen, Xiaowei Liu
doaj +1 more source
Galactic chemical evolution: Stellar yields and the initial mass function [PDF]
, 2015 We present a set of 144 Galactic chemical evolution models applied to a Milky Way analogue, computed using four sets of low+intermediate star nucleosynthetic yields, six massive star yield compilations, and six functional forms for the initial mass ...
Cavichia, Oscar +4 more
core +5 more sources
The Rapid Onset of Stellar Bars in the Baryon-dominated Centers of Disk Galaxies
The Astrophysical Journal, 2023 Recent observations of high-redshift galactic disks ( z ≈ 1–3) show a strong negative trend in the dark-matter (DM) fraction f _DM with increasing baryon surface density.
Joss Bland-Hawthorn +3 more
doaj +1 more source