The story starts at the end of the nineteenth century, when gifted scientists were systematically filling in gaps in Mendeleev's table by deciphering atomic ... in the emission spectrum of a ...

Infrared astronomy has revealed so much about the universe, ranging from protoplanetary disks and nebulae to brown dwarfs, ...

A set of eleven U atomic emission lines, between 421.099 and 421.460 nm ... for their efficacies to extract the enrichment information from the measured LIBS spectra. Wavelength-dependent weight ...

laser pulses in the near-infrared spectrum. These ultra-short bursts of light create tiny charge oscillations and atomic displacements in the water, which trigger the emission of visible light. This ...

laser pulses in the near-infrared spectrum. These ultra-short bursts of light create tiny charge oscillations and atomic displacements in the water, which trigger the emission of visible light.

researchers from Madrid explain why the angular profile of light emission depends on the step’s orientation: in cavities as small as those between the tip and the STM sample, an atomic size ...

That energy tears atoms apart into a plasma of detached electrons and atomic nuclei, reminiscent of the early Universe ...

These objects are the cores of massive stars that have gone supernova, collapsing into hot, ultradense masses so squished together they behave a lot like a single atomic nucleus the ... powerful beams ...

According to a study published in Science Advances, researchers from Madrid explain why the angular profile of light emission ...

Researchers analyze the picoantenna-like directional behaviour of tunnel junctions formed by surface defects at the atomic ...