Left: The Hubble Space Telescope captured this view, just 7 arcseconds wide, of HE0450–2958, a quasar 5 billion light-years distant in the constellation Caelum. Right: Mathematically removing most of the quasar's starlike glow enhanced the view of a neighboring galaxy (A), and it should have revealed a host galaxy surrounding the quasar (B). But it only revealed a lopsided blob of gas (C) that is entirely devoid of stars.
Courtesy NASA, ESA, and Pierre Magain (University of Liege, Belgium).
Discovered four decades ago, quasars are starlike pinpricks
of light that shine across billions of light-years of
intergalactic space. Conventional wisdom states that they
are the ultracompact, ultraluminous nuclei of massive
galaxies. The Hubble Space Telescope has amply buttressed that paradigm, showing that most of these ultraluminous beacons do inhabit recognizable galaxies. But a new Hubble study of 20 relatively nearby quasars in today's issue of
Nature has turned up one that apparently is galaxy-free.
And that poses a puzzle. After all, astronomers have
concluded that a quasar lights up because a supermassive
black hole in a galaxy's very core has gobbled up nearby
material, heating some to multimillion-degree temperatures
and blasting the rest into space at near-light speeds. If
HE0450–2958 truly lives in intergalactic space, then
astronomers have to explain where it gets its fuel.
One piece to the puzzle may be the unusual galaxy that
lies to the southeast of the ostensibly "naked" quasar. That
distorted galaxy reminds astronomer Georges Meylan (Swiss Federal Institute of Technology Lausanne) of "The Antennae" (NGC 4038 and NGC
4039), a relatively nearby pair of colliding galaxies
in Corvus. HE0450–2958 "may be a case where the original host galaxy, if there was one, was disturbed by a dynamical encounter" with the neighboring galaxy, says Meylan.
That Hubble is capable of detecting a quasar's host galaxy is evidenced by this image of HE1239–2426, 1.5 billion light-years from Earth on the Hydra-Corvus border. This quasar — presumably a supermassive black hole whose gravity accelerates surrounding matter to near-light speeds — is surrounded by a recognizable spiral galaxy.
Courtesy NASA, ESA, and Pierre Magain (University of Liege, Belgium).
Meylan, lead author Pierre Magain (University of Liege,
Belgium), and their colleagues "do seem to have done the
analysis carefully" in today's
Nature paper, says University of Arizona quasar expert Jill Bechtold — an important consideration when the analysis involves mathematically removing the quasar's far brighter light to look for details that even Hubble can only barely resolve. But that doesn't necessarily mean that HE0450–2958 is a homeless black hole, says longtime quasar observer George Djorgovski (Caltech). "Much of the host may be obscured by dust," he notes, as sometimes is the case for the host galaxies of distant gamma-ray bursts. Alternatively, the host could be a so-called
low-surface-brightness galaxy — a distant analog of the large but diffuse spirals that astronomers discovered in our cosmic backyard only recently. At HE0450–2958's considerable distance, a spread-out spiral host wouldn't register even on Hubble's sensitive detectors.
