... problem and help reduce the predicted abundances of 3He. First, some researchers suggest that the 3He formed inside the core of the stars is destroyed before the star has chance to pulsate and eject its material into...
...- and mid-infrared light only (from 0.6 to 28 micrometers). Infrared light is especially important as it will help reveal the first stars and galaxies that formed after the Big Bang. It is also at infrared wavelengths that researchers are able...
... most obvious way to make primordial SMBH seeds is from the collapse of the hypothesised very first stars - Population III stars – in the early Universe (see https://room.eu.com/news/Using_gravitational_waves...). By a combination of either mergers...
.... The team has worked incredibly hard, and the first data will reveal how well the instrument truly performs,”...thought to have lasted several hundred million years before the first stars were born. Its “dark” description is poignant both figuratively...
... that spans a wide range of wavelengths thus allowing astronomers to study a diverse area of astronomical phenomena from the first stars and galaxies that emerged from the cosmic "dark ages" billions of years ago to mapping the gas...
... in the infrared band of the electromagnetic spectrum. This will allow the telescope to look not only at the first stars and galaxies that formed after the Big Bang, but also into heavily clouded regions, that...