A water-vapour giga-maser in the active galaxy TXFS2226-184.
Active galactic nuclei are thought to be powered by gas falling into a massive black hole; the different types of active galaxy may arise because we view them through a thick torus of molecular gas at varying angles of inclination. One way to determine whether the black hole is surrounded by a torus, which would obscure the accretion disk around the black hole along certain lines of sight, is to search for water masers, as these exist only in regions with plentiful molecular gas. Since the first detection of an extra-galactic water maser in 1979, they have come to be associated primarily with active galaxies, and have even been used to probe the mass of the central engine. Here we report the detection of a water giga-maser in the radio galaxy TXFS2226-184. The strength of the emission supports a recently proposed theory of maser pumping that allows for even more powerful masers, which might be detectable at cosmological distances. Water masers may accordingly provide a way to determine distances to galaxies outside the usual distance ladder, providing an independent calibration of the Hubble constant.
Koekemoer
A M
AM
Mount Stromlo and Siding Spring Observatories, Australia.
Henkel
C
C
Greenhill
L J
LJ
Dey
A
A
van Breugel
W
W
Codella
C
C
Antonucci
R
R
D055580:Astronomical Phenomena; D001256:Astronomy; D013057:Spectrum Analysis; D014867:Water
D014867:Water