Dein Suchergebnis zum Thema: kramer

Radioastronomen haben 2019 das erste „Foto“ eines Schwarzen Lochs veröffentlicht. Die internationale Kollaboration Event Horizon Telescope hat dabei für die Beobachtungen der Galaxie Messier 87 acht weltweite Radioteleskope zusammengeschaltet. Im Zentrum von Messier 87 befindet sich ein supermassives Schwarzes Loch mit der Grösse von ca. 5.5 Milliarden Sonnenmassen.
Anton; Kramer, Michael; Menten, Karl M.; Britzen, Silke

Wissenschaftliche Publikationen
.; Kramer, M.; Pallanca, C.; Ransom, S.

Die Anammox-Reaktion ist ein erst in den 1990er Jahren entdeckter biochemischer Prozess von globaler Bedeutung. Die Enzyme, die diese Reaktion ermöglichen, liefern neue Einblicke in unkonventionelle Biochemie.
.; Kramer, E.

Ein internationales Team von Astronom:innen hat einen neuen Katalog mit 294 Pulsaren, die Gammastrahlung abgeben, veröffentlicht. Sie haben diese Gammapulsare und 34 Kandidaten, die auf eine Bestätigung warten, in Daten des Fermi Gamma-ray Space Telescope der NASA entdeckt. Forschende des Max-Planck-Instituts für Gravitationsphysik (Albert-Einstein-Institut) in Hannover haben 53 Pulsare zu dem Katalog beigetragen.
.; Kramer, M.; Kuss, M.; Latronico, L.; Shiu-Hang;

A European team with the participation of the Max Planck Institutes for Gravitational Physics and Radio Astronomy, together with Indian and Japanese astronomers, has discovered the first evidence of a gravitational wave background originating from the formation and evolution of the universe and its galaxies. The team used the European Pulsar Timing Array and the Indian Pulsar Timing Array to observe gravitational waves at wavelengths of several light years over a period of 25 years. The target of the observations was not gravitational waves directly, but 25 pulsar stars distributed in the Milky Way, which form the largest gravitational wave detector to date. Pulsars rotate very quickly around their axis and can be measured from Earth via periodic radio pulses that are as regular as clockwork. Gravitational waves influence the fabric of space and time. If gravitational waves meet pulsars, they can be measured indirectly via the changed clock frequency of the pulsars.
49 331 567-7303 elke.mueller@aei.mpg.de Michael Kramer

A European team with the participation of the Max Planck Institutes for Gravitational Physics and Radio Astronomy, together with Indian and Japanese astronomers, has discovered the first evidence of a gravitational wave background originating from the formation and evolution of the universe and its galaxies. The team used the European Pulsar Timing Array and the Indian Pulsar Timing Array to observe gravitational waves at wavelengths of several light years over a period of 25 years. The target of the observations was not gravitational waves directly, but 25 pulsar stars distributed in the Milky Way, which form the largest gravitational wave detector to date. Pulsars rotate very quickly around their axis and can be measured from Earth via periodic radio pulses that are as regular as clockwork. Gravitational waves influence the fabric of space and time. If gravitational waves meet pulsars, they can be measured indirectly via the changed clock frequency of the pulsars.
49 331 567-7303 elke.mueller@aei.mpg.de Michael Kramer

Nineteen observatories worldwide are carefully examining the centre of the giant galaxy M 87 at all possible wavelengths
Michael Kramer Max Planck Institute for Radio Astronomy

Scientific Publications
.; Kramer, M.; Pallanca, C.; Ransom, S.

Scientific Publications
.; Kramer, M.; Pallanca, C.; Ransom, S.

Wissenschaftliche Publikationen
.; Kramer, M.; Pallanca, C.; Ransom, S.