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A megamaser acts as an astronomical laser that beams out microwave emission rather than visible light (hence the ‘m’ replacing the ‘l’).
A megamaser acts as an astronomical laser that beams out microwave emission rather than visible light (hence the ‘m’ replacing the ‘l’).
Galaxies MCG+01-38-004 (upper) and MCG+01-38-005 (lower) – the microwave emissions from MCG+01-38-005 were used to calculate a refined value for the H
Galaxies MCG+01-38-004 (upper) and MCG+01-38-005 (lower) – the microwave emissions from MCG+01-38-005 were used to calculate a refined value for the Hubble constant.
Arp 220, the prototypical hydroxyl megamaser host galaxy (Hubble Space Telescope)
Arp 220, the prototypical hydroxyl megamaser host galaxy (Hubble Space Telescope)
The 1665 and 1667 MHz maser lines in Arp 220, which have been redshifted to lower frequencies (Arecibo Observatory data)
The 1665 and 1667 MHz maser lines in Arp 220, which have been redshifted to lower frequencies (Arecibo Observatory data)
Aurorae on the north pole of Jupiter generate cyclotron masers (Hubble)
Aurorae on the north pole of Jupiter generate cyclotron masers (Hubble)
Pulsations of the Mira variable S Orionis, showing dust production and masers (ESO)
Pulsations of the Mira variable S Orionis, showing dust production and masers (ESO)
WISE image of IC 443, a supernova remnant with maser emission
WISE image of IC 443, a supernova remnant with maser emission