Water vapour reveals how stars form around black hole

Water vapour reveals how stars form around black hole Click here for a high res image. Klik hier voor een hoge resolutie foto.

 

An international team led by astronomer Paul van der Werf (Leiden University, The Netherlands) has discovered that a black hole in the young universe is surrounded by a large disk of gas and dust, where stars form rapidly and which is so dense that light can barely escape from it. The team made this unexpected discovery during a successful search for water vapour in a galaxy in the early universe, located at a distance of 12 billion light-years.

The discovery was made using the sensitive radio telescopes of IRAM (Institut de Radioastronomie Millimétrique) at the Plateau de Bure in the French Alps. These telescopes were used to search for water vapour in a quasar, a galaxy in the early universe that derives its luminosity from the growth of a black hole hundreds of millions of times more massive than our sun. Team leader Paul van der Werf says: "Water in cosmic clouds is normally frozen to ice, but the ice can be evaporated by the strong radiation of the quasar or of young stars. Therefore we decided to search for water vapour in this object. It is located so far away that we are looking back in time, to an era where the universe was only 10% of its present age. This is one of the first searches ever conducted to find water in the early universe."

The big surprise was however not the amount of water vapour found (1000 trillion times the amount of water on Earth) but the discovery of an opaque disk in which the water vapour is located and which rapidly forms young stars. The density of the disk is so high that light barely escapes. Team member Marco Spaans (University of Groningen, The Netherlands) explains: "Water molecules are sensitive to infrared radiation, so we could use the water vapour detected as a cosmic infrared light meter. With this method we found that essentially all radiation is locked up in the gas disk surrounding the black hole. This trapped radiation is so intense that it will build up enormous pressure and eventually blow away the gas and dust clouds surrounding the black hole."

This conclusion sheds a surprising new light on the connection between black holes and the galaxies in which they reside. Team member Alicia Berciano Alba (ASTRON, The Netherlands) says: "There is a mysterious relation between the masses of black holes in the centers of galaxies and the masses of the galaxies themselves, as if the formation of both is regulated by the same process. Our results show that these opaque gas disks, which will be ultimately blown away by the intense pressure of the trapped radiation, probably play a key role in this process." IRAM director Pierre Cox, co-author of the paper, adds: "This discovery opens new possibilities for studying galaxies in the early universe, using water molecules that probe regions closest to the central black hole, that are otherwise difficult to explore."

The team is now looking for water vapour in other objects in the early universe. A paper describing this discovery is due to appear shortly in Astrophysical Journal Letters.



To the editors:

Contact information:

Paul van der Werf
Leiden Observatory
Leiden University, The Netherlands
pvdwerf [at] strw [dot] leidenuniv [dot] nl
Telephone: (+31) 71 5275883

Alicia Berciano Alba
ASTRON
Dwingeloo, The Netherlands
berciano [at] astron [dot] nl
Telephone: (+31) 521 595775

Marco Spaans
Kapteyn Institute
University of Groningen, The Netherlands
spaans [at] astro [dot] rug [dot] nl
Telephone: (+31) 50 3634092

Pierre Cox
Institut de Radioastronomie Millimétrique
Grenoble, France
cox [at] iram [dot] fr
Telephone: (+33) 476 824953

Image:

Artist impression of the gas and dust disk discovered. The inner region of the disk is heated by energy generated by the growth of the central black hole. The disk is so dense that even radiation can barely escape. (Credit: NASA/JPL-Caltech)

Images of the IRAM telescopes used:
http://www.iram.fr/EN/photo-gallery.php

Research team:

P.P. van der Werf (Leiden Observatory, Leiden University, The Netherlands)
A. Berciano Alba (ASTRON, Dwingeloo, The Netherlands
& Leiden Observatory, Leiden University, The Netherlands)
M. Spaans (Kapteyn Institute, University of Groningen, The Netherlands)
A.F. Loenen (Leiden Observatory, Leiden University, The Netherlands)
R. Meijerink (Leiden Observatory, Leiden University, The Netherlands)
D. Riechers (California Institute of Technology, Pasadena, Califonia, USA)
P. Cox (Institut de Radioastronomie Millimétrique, Grenoble, France)
A. Weiß (Max-Planck-Institut für Radioastronomie, Bonn, Germany)
F. Walter (Max-Planck-Institut für Astronomie, Heidelberg, Germany)

On-line pre-publication:

Water vapor emission reveals a highly obscured, star forming nuclear region in the QSO host galaxy APM 08279+5255 at z=3.9. Van der Werf, P.P., Berciano Alba, A., Spaans, M., Loenen, A.F., Meijerink, R., Riechers, D.A., Cox, P., Weiß, A., & Walter, F.
Astrophysical Journal Letters, in press http://arxiv.org/abs/1106.4825  

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