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"More than 20 years of regular high precision timing with Effelsberg and other radio telescopes of the European Pulsar Timing Array and the North American NANOGrav pulsar timing projects showed with high precision that there is no change in the eccentricity of the orbit," explains Norbert Wex, also from MPIfR. "This means that to a high degree the neutron star feels the same kind of attraction towards dark matter as towards other forms of standard matter."
We're looking all the way through the Milky Way, past its center, way out into the other side," MPIfR's Karl Menten said in the statement.
"Similar observations with ALMA will become increasingly common, and more and more detailed images showing inhomogeneous structures in disk density become available," says Karl Menten, director at MPIfR and a co-author of the paper, in a statement.
Jansky Very Large Array (VLA), and the MPIfR's 100-meter Effelsberg radio telescope in Germany.
Using ingenious data analysis methods, researchers from the Max Planck Institutes for Gravitational Physics (MPG) and for Radio Astronomy (MPIfR), in an international collaboration, dug a very special gamma-ray pulsar out of data from the Fermi Gamma-ray Space Telescope.
The present project brings together the expertise of two research groups at MPIfR, infrared interferometry in order to investigate the structure of the disk and submillimeter astronomy showing the structure of the bipolar outflow," he added.
Led by Keiichi Ohnaka at the Max Planck Institute for Radio Astronomy (MPIfR) in Bonn, the astronomers, for the first time showed how the gas is moving in different areas over the surface of a distant star known as Betelgeuse.
Byrd Green Bank Telescope (GBT), and the Effelsberg Radio Telescope of the Max Planck Institute for Radioastronomy (MPIfR) in Germany to determine that a galaxy dubbed UGC 3789 is 160 million light-years from Earth.
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