An article in publication and an article under peer-review in “The Astrophysical Journal” report various aspects of a study of 6 so-called jellyfish galaxies. A team of researchers used various instruments to examine them and try to understand the processes taking place in the “tentacles” generated by the gas stripped from those galaxies during the passage within a galaxy cluster. In that space, there’s intergalactic plasma that generates a pressure that caused that gas loss in a process called ram pressure stripping. An image of the jellyfish galaxy cataloged as JO201 captured by the Hubble Space Telescope was published by ESA.
A few hours ago the Soyuz MS-23 spacecraft docked with the International Space Station. It blasted off on Friday, February 24, with the aim to replace the Soyuz MS-22, which use in safety conditions was made impossible by a failure in its cooling system. Now the mission of Dmitri Petelin, Frank Rubio, and Sergey Prokopyev could be extended for a total duration of about a year using the Soyuz MS-23 to enable them to come back to Earth.
A few hours ago, the Soyuz MS-23 spacecraft blasted off atop a Soyuz-2.1a rocket from the Baikonur Cosmodrome, Kazakhstan. After about nine minutes it successfully separated from the rocket’s last stage and was placed on its route, which requires about two days of journey. It replaces the damaged Soyuz MS-22 as a vehicle for the return of its three crew members: Dmitri Petelin, Frank Rubio, and Sergey Prokopyev. This is the solution chosen by the Russian Roscosmos space agency after having established the impossibility of using the Soyuz MS-22 for the return journey with a crew on board in safety conditions.
An article being published in “The Astrophysical Journal” reports the results of the study of two galaxy mergers between dwarf galaxies with active galactic nuclei. A team of researchers used data collected by NASA’s Chandra X-ray Observatory to discover candidates and then compared them with infrared observations conducted with NASA’s WISE Space Telescope and optical frequency observations conducted with the Canada-France-Hawaii Telescope (CFHT).
An article published in “The Astrophysical Journal” reports the results of twenty years of observations of a giant filament of gas and dust that is progressively approaching Sagittarius A*, the supermassive black hole at the center of the Milky Way. A team of researchers from the Keck Observatory and UCLA’s Galactic Center Orbits Initiative (GCOI) used Keck’s OSIRIS and NIRC2 instruments to keep an eye on this filament, cataloged as X7, to study its orbit and shape’s evolution. According to predictions, in 2036, X7 will get close to Sagittarius A* to the point of dissipating and be devoured. This will be a really interesting event to study even more deeply what happens in that really extreme environment.