«We expected the burster to act at
radio wavelengths much as it does at X-ray and visible wavelengths — that is, rise in brightness, then slowly become weaker,» said Dr. Dale Frail of the National Radio Astronomy Observatory (NRAO).
Not exact matches
In the hopes of seeing the gas clouds from which the first stars arose, Loeb has devoted
much of the past decade to a new field called 21 - centimeter cosmology, a branch of
radio astronomy that focuses on identifying electromagnetic radiation that started out with a
wavelength of 21 centimeters.
Some, with
much longer
wavelengths than we can see, would transform the world:
radio waves.
Its dishes collect
wavelengths about a millimeter or less —
much shorter than those detected by traditional
radio telescopes.
This unprecedented image of Herbig - Haro object HH 46/47 combines
radio observations acquired with the Atacama Large Millimeter / submillimeter Array (ALMA) with
much shorter
wavelength visible light observations from ESO's New Technology Telescope (NTT).
Hallinan is planning continued
radio observations over the next year or two, because this
radio emission — which will be around long after all of the other
wavelengths have faded — is the most important diagnostic of the energetics and environment of the explosion, and may reveal how
much energy was in the explosion, how
much mass was ejected, if a jet actually appeared, and if the merger produced conditions that will influence future star formation, among other questions.
In deep space,
much material is
much colder, and emits at even lower
wavelengths, down in the
radio bands.