Press Release 09-02-05 Press Releases 2009

Infant Galaxies: Small and Hyperactive

When galaxies are born, do their stars form everywhere at once, or only within a small core region? Recent measurements provide the first concrete evidence that star-forming regions in infant galaxies are indeed small – but also hyperactive, producing stars at astonishingly high rates.

This is the conclusion drawn from recent observations of one of the most distant known galaxies: a so-called quasar with the designation J1148+5251. Light from this galaxy takes 12.8 billion years to reach Earth; in turn, astronomical observations show the galaxy as it appeared 12.8 billion years ago, providing a glimpse of the very early stages of galactic evolution, less than a billion years after the Big Bang.

The observers, an international team of researchers led by scientists from the Max Planck Institute for Astronomy, made use of the IRAM Interferometer, a German-French-Spanish radio telescope, to obtain images of a very special kind: They recorded the infrared radiation emitted by J1148+5251 at a specific frequency associated with ionized carbon atoms, which is a reliable indicator of ongoing star formation. The resulting images show sufficient detail to allow, for the first time, the measurement of the size of a very early star-forming region. With this information, the researchers were able to conclude that, at the time, stars were forming in the core region of J1148+5251 at record rates – any faster, and star formation would have been in conflict with the laws of physics.

The results will be published in the February 5 issue (Volume 457, No. 7230) of the journal Nature.

„This galaxy's rate of star production is simply astonishing,“ says the article's lead author, Dr Fabian Walter of the Max Planck Institute for Astronomy. „Every year, this galaxy's central region produces new stars with the combined mass of more than a thousand suns." By contrast, the rate of star formation within our own galaxy, the Milky Way, is roughly one solar mass per year.

Close to the (physical) limit
It has been known for some time that young galaxies can produce impressive amounts of new stars, but overall activity is only part of the picture. Without knowing the star-forming region's size, it is impossible to compare star formation in early galaxies with theoretical models, or with star-forming regions in our own galaxy.

With a diameter of a mere 4000 light-years (for comparison: the Milky Way galaxy's diameter amounts to 100.000 light-years), the star-forming core of J1148+5251 is extremely productive. In fact, it is close to the limits imposed by physical law! Stars are formed when cosmic clouds of gas and dust collapse under their own gravity. As the clouds collapse, temperatures rise, and internal pressure starts to build. Once that pressure has reached certain levels, all further collapse is halted, and no additional stars can form. The result is an upper limit on how many stars can form in a given volume of space in a given period of time.

Remarkably, the star-forming core of J1148+5251 reaches this absolute limit. Fabian Walter: „This extreme level of activity can be found in parts of our own galaxy, but only on much smaller scales. For example, there is a region within the Orion nebula that is just as active as what we have observed. But in J1148+5251, we are dealing with what amounts to a hundred million of these smaller regions combined!“ Earlier observations of different galaxies had suggested an upper limit that amounts to a tenth of the value now observed in J1148+5251.

Abbildung 1  
Figure 1: False-color image of the galaxy J1148+5251. Based on observations with the Very Large Array in New Mexico.

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  Figure 2: The level of star-forming activity in the Orion-KL region (marked by the rectangle) in the Orion nebula is comparable to that of the central region of J1148+5251, but confined to a much smaller volume of space.
(NASA, ESA, Robberto (STScI/ESA), Orion Treasury Project Team)

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Growth from within
The compact star-forming region of J1148+5251 provides a highly interesting data point for researchers modeling the evolution of young galaxies. Going by this example, galaxies grow from within: In the early stages of star formation, there is a core region in which stars form very quickly. Presumably, such core regions grow over time, mainly as a result of collisions and mergers between galaxies, resulting in the significantly larger star-filled volume of mature galaxies.

A dime at 8.5 miles
The key to these results is one novel measurement: the first resolved image of an extremely distant quasar's star-forming central region, clearly showing the region's apparent diameter, and thus its size. This measurement is quite a challenge in itself. At a distance of almost 13 billion light-years (corresponding to a red-shift z = 6.42), the star-forming region, with its diameter of 4000 light-years, has an angular diameter of 0.27 seconds of arc – the size of a dime, viewed at a distance of roughly 9 miles (or a pound coin, viewed at a distance of roughly 11 miles).

There is one further handicap: The observations rely on electromagnetic radiation with a characteristic wavelength, which is associated with ionized carbon atoms. At this wavelength, the star-forming regions of J1148+5251 outshine even the quasar's ultra-bright core. Due to the fact that the universe is expanding, the radiation is shifted towards longer wavelengths as it travels towards Earth („cosmological redshift“), reaching our planet in the form of radio waves with a wavelength of about one millimeter. But, owing to the general nature of waves, it is more than a thousand times more difficult to resolve minute details at a wavelength of one millimeter, compared with visible light.

Observations at the required wavelength and level of detail became possible only as recently as 2006, thanks to an upgrade of the German-French-Spanish IRAM Interferometer, a compound radio telescope on the Plateau de Bure in the French Alps.

Abbildung 4   Abbildung 3
Figure 3: Radio telescopes of the IRAM Interferometer on the Plateau de Bure in the French Alps.

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  Figure 4: Four antennas of RAM on top of the Plateau de Bure.

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Future telescopes
Use of the characteristic radiation of ionized carbon to detect and image star-forming regions in extremely distant had been suggested some time ago. A significant portion of the observational program for ALMA, a compound radio telescope currently under construction in Northern Chile, relies on this observational approach. But up until the measurements of Fabian Walter and his colleagues, this technique had not been demonstrated in practice. Quoting Walter: „The early stages of galaxy evolution, roughly a billion years after the Big Bang, will be a major area of study for years to come. Our measurements open up a new window on star-forming regions in very young galaxies.“

Institutions involved in this collaboration:
Max Planck Institute for Astronomy, Heidelberg, Germany
Argelander Institute for Astronomy, Bonn, Germany
Max Planck Institute for Radio Astronomy, Bonn, Germany
California Institute of Technology, Pasadena, USA
Institut de Radio Astronomie Millimetrique, Saint Martin d’Herès, France
Istituto Nazionale di Astrofisica, Osservatorio di Roma, Italy
National Radio Astronomy Observatory, Socorro, USA

Contact persons:
Dr. Fabian Walter   Tel.: 06221 – 528 225
Dr. Jakob Staude   Tel.: 06221 – 528 229
Dr. Markus Pössel   Tel.: 06221 – 528 261

For further information as well as images, please visit:
Hintergrundinformation Hi-Tech und Schützenhilfe vom Universum

Press Releases 2009 German version of this Press Release
(includes further background information)

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  PR090205_2o.pdf PDF 1.6 MB RGB Without Frame AI 28.8 MB CMYK Adobe Illustrator
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