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Close-up view of galaxies prompts re-think on star formation

Date:
November 10, 2015
Source:
University of Edinburgh
Summary:
Astronomers have identified for the first time one of the key components of many stars, a study suggests. A type of gas found in the voids between galaxies -- known as atomic gas -- appears to be part of the star formation process under certain conditions, researchers say.
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Astronomers have identified for the first time one of the key components of many stars, a study suggests.

A type of gas found in the voids between galaxies -- known as atomic gas -- appears to be part of the star formation process under certain conditions, researchers say.

The findings overturn a long-standing theory about the conditions needed for star formation to take place -- a process that happens when dense clouds of dust and gas inside galaxies collapse.

It was previously thought that stars could form only in the presence of a different type of gas -- called molecular gas.

Atomic gas is composed of individual hydrogen atoms. It is usually found in regions of space that do not contain any planets or stars and are largely empty, researchers say.

Molecular gas is made up of pairs of hydrogen atoms bound together, and is present in the densest parts of galaxies, where most planets and stars form.

The new study, led by the University of Edinburgh, provides the first evidence that atomic gas can fuel star formation. This happens when atomic gas flows into galaxies but does not have time to convert to the molecular form, the team says.

The discovery was made by studying galaxies in which explosions of massive stars -- known as gamma-ray bursts -- have been observed. It was thought the stars formed from molecular gas, but recent studies have shown these galaxies to be almost entirely deficient in molecular gas.

Using a radio telescope in New South Wales, Australia, researchers measured the levels of atomic gas present in the galaxies. The team found they contain large amounts of atomic gas, distributed close to gamma-ray bursts, suggesting it can act as the fuel for star formation.

Stars form in the same way regardless of the type of gas involved, scientists say. Gas molecules are destroyed early in the process, so the stars they produce are the same, they add.

The study, published in the journal Astronomy & Astrophysics, was funded by the Science and Technology Facilities Council. The research was carried out in collaboration with researchers at institutions across Europe, the US and Australia.

Dr Michal Michalowski, of the University of Edinburgh's School of Physics and Astronomy, who led the study, said: "We were analysing the atomic gas data for these galaxies when the results about their molecular gas deficiency were announced. We pieced together all the information, and found that stars may in fact form out of atomic gas, which was previously believed to be impossible."


Story Source:

Materials provided by University of Edinburgh. Note: Content may be edited for style and length.


Journal Reference:

  1. A. Nicuesa Guelbenzu, S. Klose, E. Palazzi, J. Greiner, M. J. Michałowski, D. A. Kann, L. K. Hunt, D. Malesani, A. Rossi, S. Savaglio, S. Schulze, D. Xu, P. M. J. Afonso, J. Elliott, P. Ferrero, R. Filgas, D. H. Hartmann, T. Krühler, F. Knust, N. Masetti, F. Olivares E., A. Rau, P. Schady, S. Schmidl, M. Tanga, A. C. Updike, K. Varela. Identifying the host galaxy of the short GRB 100628A. Astronomy & Astrophysics, 2015; 583: A88 DOI: 10.1051/0004-6361/201425160

Cite This Page:

University of Edinburgh. "Close-up view of galaxies prompts re-think on star formation." ScienceDaily. ScienceDaily, 10 November 2015. <www.sciencedaily.com/releases/2015/11/151110094028.htm>.
University of Edinburgh. (2015, November 10). Close-up view of galaxies prompts re-think on star formation. ScienceDaily. Retrieved May 26, 2017 from www.sciencedaily.com/releases/2015/11/151110094028.htm
University of Edinburgh. "Close-up view of galaxies prompts re-think on star formation." ScienceDaily. www.sciencedaily.com/releases/2015/11/151110094028.htm (accessed May 26, 2017).

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