Results 171 to 180 of about 205,088 (284)

Cosmic Rays and the Askaryan Effect Reveal Subsurface Structure and Buried Ice on the Moon

open access: yesGeophysical Research Letters, Volume 52, Issue 6, 28 March 2025.
Abstract We present the first full‐wavelength numerical simulations of the electric field generated by cosmic ray impacts into the Moon. Billions of cosmic rays fall onto the Moon every year. Ultra‐high energy cosmic ray impacts produce secondary particle cascades within the regolith and subsequent coherent, wide‐bandwidth, linearly‐polarized radio ...
E. S. Costello   +12 more
wiley   +1 more source

First constraints on iron abundance versus reflection fraction from the Seyfert 1 galaxy MCG-6-30-15 [PDF]

open access: bronze, 1999
Julia C. Lee   +4 more
openalex   +1 more source

Stellar abundances of early-type galaxies [PDF]

open access: yes, 2008
It is currently impossible to determine the abundances of stellar populations star-by-star in dense stellar systems more distant than a few megaparsecs. Therefore, methods to analyse the composite light of stellar systems are required. I review recent progress in determining the abundances and abundance ratios of early-type galaxies.
openaire   +3 more sources

On the Evolutionary History of a Simulated Disk Galaxy as Seen by Phylogenetic Trees

open access: yesThe Astrophysical Journal
Phylogenetic methods have long been used in biology and more recently have been extended to other fields—for example, linguistics and technology—to study evolutionary histories.
Danielle de Brito Silva   +14 more
doaj   +1 more source

Chemical abundances and ionizing clusters of H ii regions in the LINER galaxy NGC 4258 [PDF]

open access: bronze, 2000
Á. I. Díaz   +3 more
openalex   +2 more sources

Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys

open access: yesThe Astrophysical Journal
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

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