Results 91 to 100 of about 52,093 (177)
Next-generation surveys are expected to uncover thousands of globular cluster (GC) stellar streams, motivating the need for a theoretical framework that produces realistic GC streams in a fully cosmological, Milky Way–like environment.
Nondh Panithanpaisal +9 more
doaj +1 more source
Preemptive iodide treatment in the event of a nuclear disaster: The prepper's guide to the galaxy
Experimental Physiology, Volume 110, Issue 12, Page 1771-1776, December 1, 2025.
Per Karkov Cramon +2 more
wiley +1 more source
A deep understanding of our Galaxy calls for detailed decomposition of its stellar populations via their chemical fingerprints. This requires precise stellar abundances of many elements for a large number of stars.
Meng Zhang +13 more
doaj +1 more source
Unlocking all the physical information encoded in low-resolution spectra poses a significant challenge for astronomical survey analysis. Such a task demands modeling spectra and optimizing astrophysical parameters in high-dimensional space as a ...
Tianmin Wu +6 more
doaj +1 more source
Properties of the Magellanic Corona
We characterize the Magellanic Corona, the warm gaseous halo around the Large Magellanic Cloud (LMC). The Corona is a key ingredient in the formation of the Magellanic Stream and has recently been observed in high-ion absorption around the LMC.
Scott Lucchini +2 more
doaj +1 more source
Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
The abundance of faint dwarf galaxies is determined by the underlying population of low-mass dark matter (DM) halos and the efficiency of galaxy formation in these systems. Here, we quantify potential galaxy formation and DM constraints from future dwarf
Ethan O. Nadler +6 more
doaj +1 more source
2022 この博士論文は内容の要約のみの公開(または一部非公開 ...
openaire +1 more source
Very-metal-poor stars ([Fe/H] < −2) are important laboratories for testing stellar models and reconstructing the formation history of our galaxy. Asteroseismology is a powerful tool to probe stellar interiors and measure ages, but few asteroseismic ...
Daniel Huber +17 more
doaj +1 more source
Characterizing the 3D Structure of Molecular Cloud Envelopes in the Cloud Factory Simulations
We leverage recent numerical simulations of highly resolved star-forming regions in a Milky Way–like galaxy to explore the nature of extended gaseous envelopes around molecular clouds.
Elijah Mullens +3 more
doaj +1 more source

