Results 101 to 110 of about 553,339 (197)
We present the first high-resolution abundance study of ESO 280-SC06, one of the least luminous and most metal-poor gravitationally bound Milky Way globular clusters.
Sam A Usman +8 more
doaj +1 more source
Identification of specific stellar populations using photometry for spectroscopic follow-up is a first step to confirm and better understand their nature.
F. Quispe-Huaynasi +15 more
doaj +1 more source
The Origin of Young Stellar Populations in NGC 1783: Accretion of External Stars
The presence of young stellar populations in the Large Magellanic Cloud cluster NGC 1783 has caught significant attention, with suggestions ranging from it being a genuine secondary stellar generation to a population of blue straggler stars or simply ...
Li Wang +6 more
doaj +1 more source
Observations of Extremely Metal-poor O Stars: Weak Winds and Constraints for Evolution Models
Metal-poor massive stars drive the evolution of low-mass galaxies, both locally and at high redshift. However, quantifying the feedback they impart to their local surroundings remains uncertain because models of stellar evolution, mass loss, and ionizing
O. Grace Telford +5 more
doaj +1 more source
The rotation of low mass stars at 30 Myr in the cluster NGC 3766. [PDF]
Roquette J +6 more
europepmc +1 more source
Low-mass neutron star nucleosynthesis — stripping scenario
This paper examines nucleosynthesis in a low-mass neutron star crust that loses mass due to accretion in a close binary system and reaching a hydrodynamically unstable configuration explodes. The r-process proceeds mainly in the inner crust. Nucleosynthesis in the outer crust is an explosive process with a sharp increase in temperature caused by an ...
A. Yu. Ignatovskiy +2 more
openaire +2 more sources
Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]
Cang T +13 more
europepmc +2 more sources
Wind Roche-lobe Overflow in Low-mass Binaries: Exploring the Origin of Rapidly Rotating Blue Lurkers
Wind Roche-lobe overflow (WRLOF) is a mass-transfer mechanism proposed by Mohamed and Podsiadlowski for stellar binaries wherein the wind acceleration zone of the donor star exceeds its Roche-lobe radius, allowing stellar wind material to be transferred ...
Meng Sun +6 more
doaj +1 more source
Characterizing <i>K2</i> Candidate Planetary Systems Orbiting Low-Mass Stars IV: Updated Properties for 86 Cool Dwarfs Observed During Campaigns 1-17. [PDF]
Dressing CD +17 more
europepmc +1 more source

