At these wavelengths, astronomers can peer at the disks of gas and dust around newborn stars, see into star - forming clouds, and observe early galaxies that are bright in submillimetre wavelengths but obscured by dust in optical ligh
At these
wavelengths, astronomers can peer
at the disks of gas and dust around newborn stars, see into star - forming clouds, and observe early galaxies that are bright in submillimetre wavelengths but obscured by dust in optical ligh
at the disks of gas and dust around newborn stars, see into star - forming clouds, and observe early galaxies that are
bright in submillimetre
wavelengths but obscured by dust in
optical light.
The cocoon also explains other details of the event, such as the initial
bright blue flash observed
at ultraviolet and
optical wavelengths, and the delay in the appearance of X-rays and radio waves.