A team of researchers with affiliations to multiple institutions in the U.S. has found that the metal content of Fermi bubble high-velocity clouds does not match with material in the Milky Way’s galactic center, suggesting that at least some of the material comes from somewhere else. In their paper published in the journal Nature Astronomy, the group describes their analysis of the makeup of the clouds and their conclusions.

Prior research has shown that massive lobes of plasma extend above and below the center of the galactic plane that forms the Milky Way galaxy. Prior research has also suggested that the lobes are globular gas formations which has led to their nickname—Fermi bubbles...

Yale scientists have developed a novel omicron-specific mRNA vaccine that offers superior immune protection against two viral subvariants than standard mRNA vaccines.

The new vaccine, called Omnivax, increased neutralizing antibody response against the BA.1 and BA.2.12.1 omicron subvariants in pre-immunized mice 19-fold and eight-fold, respectively, compared with standard mRNA vaccines. The improved response against the BA.1 subvariant was reported June 6 in the journal Nature Communications. The results of the study involving the BA.2 subvariant were published July 19 in the journal Cell Discovery.

“While standard mRNA vaccines still offer protection against infection from new variants, their effectiveness wanes over time and was compromised due...

Passive day cooling is a promising technology for the sustainable reduction of energy consumption. It avoids the heating up of buildings by solar radiation and dissipates accumulated heat without external energy consumption. Researchers at the University of Bayreuth have now created a test system with which the materials used for passive cooling can be reliably characterised and compared — regardless of weather conditions and environmental conditions...

Astronomers at the University of Arizona have developed a theory to explain the presence of the largest molecules known to exist in interstellar gas.

The team simulated the environment of dying stars and observed the formation of buckyballs (carbon atoms linked to three other carbon atoms by covalent bonds) and carbon nanotubes (rolled up sheets of single-layer carbon atoms). The findings indicate that buckyballs and carbon nanotubes can form when silicon carbide dust—known to be proximate to dying stars—releases carbon in reaction to intense heat, shockwaves and high energy particles.

“We know from infrared observations that buckyballs populate the interstellar medium,” said Jacob Bernal, who led the research...