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Primeri s interneta (nije provereno)

mit ähnlicher Masse, Größe und Entfernung, aber normalem Gasgehalt.

Ihr wichtigstes Instrument hierbei war das Westerbork Synthesis Radio Telescope ( WSRT ) ergänzt durch aufwändige Computersimulationen ( Aktuelle Forschung : Mai 2013 ) .

In den letzten drei Jahrzehnten gab es bereits etliche Versuche, die Verteilung des kalten atomaren Gases in Galaxien mit Radio-Synthese-Teleskopen zu vermessen.

www.mpa-garching.mpg.de

Therefore, an international group of scientists at MPA and ASTRON in the Netherlands joined forces and carried out the Bluedisk project to map neutral hydrogen in a sample of 25 very gas-rich galaxies as well as a similar-sized sample of “ control ” galaxies with similar masses, sizes and distances, but normal gas content.

Their main tools were the Westerbork Synthesis Radio Telescope ( WSRT ) as well as elaborate computer simulations ( see Research Highlight May 2013 ) .

There have been many efforts over the past three decades to map the distribution of cold, atomic gas in galaxies using radio synthesis telescopes.

www.mpa-garching.mpg.de

Primeri s interneta (nije provereno)

Therefore, an international group of scientists at MPA and ASTRON in the Netherlands joined forces and carried out the Bluedisk project to map neutral hydrogen in a sample of 25 very gas-rich galaxies as well as a similar-sized sample of “ control ” galaxies with similar masses, sizes and distances, but normal gas content.

Their main tools were the Westerbork Synthesis Radio Telescope ( WSRT ) as well as elaborate computer simulations ( see Research Highlight May 2013 ) .

There have been many efforts over the past three decades to map the distribution of cold, atomic gas in galaxies using radio synthesis telescopes.

www.mpa-garching.mpg.de

mit ähnlicher Masse, Größe und Entfernung, aber normalem Gasgehalt.

Ihr wichtigstes Instrument hierbei war das Westerbork Synthesis Radio Telescope ( WSRT ) ergänzt durch aufwändige Computersimulationen ( Aktuelle Forschung : Mai 2013 ) .

In den letzten drei Jahrzehnten gab es bereits etliche Versuche, die Verteilung des kalten atomaren Gases in Galaxien mit Radio-Synthese-Teleskopen zu vermessen.

www.mpa-garching.mpg.de

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