Not exact matches
Previously, astronomers have used x-ray telescopes to observe strong winds very near the massive black holes
at galactic centers (artist's concept, inset) and
infrared wavelengths to
detect the vast outflows of cool gas (bluish haze in artist's concept, main image) from such galaxies as a whole, but they've never done so in the same galaxy.
[10] A compact radio source was found
at the centre of this nebula, and an
infrared point source has also been found, but it has not been
detected at optical
wavelengths.
However, ground - based telescopic observations
at infrared wavelengths have not yet
detected the planet.
This excess emission has been suggested to stem from debris di... ▽ More (abridged)
Infrared excesses associated with debris disk host stars
detected so far peak
at wavelengths around ~ 100 -LCB- \ mu -RCB- m or shorter.
We have clearly
detected FIR dust emission extended in the halo of the galaxy; there are two filamentary emission structures extending from the galactic disk up to 9 kpc in the northern and 6 kpc in the northwestern direct... ▽ More We present new far -
infrared (FIR) images of the edge - on starburst galaxy NGC253 obtained with the Far - Infrared Surveyor (FIS) onboard AKARI at wavelengths of 90 um and
infrared (FIR) images of the edge - on starburst galaxy NGC253 obtained with the Far -
Infrared Surveyor (FIS) onboard AKARI at wavelengths of 90 um and
Infrared Surveyor (FIS) onboard AKARI
at wavelengths of 90 um and 140 um.
After a series of brief studies by
infrared instruments carried on sounding rockets had
detected about 4,000 celestial sources of
infrared radiation, the United States, the United Kingdom, and the Netherlands built IRAS to map the sky
at infrared wavelengths of 12, 25, 60, and 100 micrometres.