Die NASA verfolgt supermassereiche Schwarze Löcher in ihrem Kollisionszyklus
- Milky Way, likely formed larger galaxies through collisions in the early Universe.
- These newly-discovered merging dwarf galaxies can be used as analogs for more distant ones that are too faint to observe.
- The dwarf galaxies are on collision courses and are found in the galaxy clusters Abell 133 and Abell 1758S.
A new study using NASA’s Chandra X-ray Observatory has tracked two pairs of supermassive black holes in dwarf galaxies on collision courses. This is the first evidence for such an impending encounter, providing scientists with important information about the growth of black holes in the early Universe.
By definition, dwarf galaxies contain stars with a total mass less than 3 billion Suns — or about 20 times less than the Milky Way. Astronomers have long suspected that dwarf galaxies merge, particularly in the relatively early Universe, in order to grow into the larger galaxies seen today. However, current technology cannot observe the first generation of dwarf galaxy mergers because they are extraordinarily faint at their great distances. Another tactic — looking for dwarf galaxy mergers closer by — had not been successful to date.
Die neue Studie überwand diese Herausforderungen, indem sie eine systematische Untersuchung von Chandras Tiefenröntgenbeobachtungen durchführte und sie mit Infrarotdaten des Wide Infrared Survey Explorer (WISE) der NASA und optischen Daten des Canada, France and Hawaii Telescope (CFHT) verglich.
Chandra war in dieser Studie besonders wertvoll, da das Material, das schwarze Löcher umgibt, auf Millionen Grad erhitzt werden kann und große Mengen an Röntgenstrahlen abgibt. Das Team suchte nach Paaren heller Röntgenquellen in kollidierenden Zwerggalaxien als Beweis für zwei Schwarze Löcher und entdeckte zwei Beispiele.
Ein Paar befindet sich im Galaxienhaufen Abell 133, der sich 760 Millionen Lichtjahre von der Erde entfernt befindet und im zusammengesetzten Bild links zu sehen ist. Chandra-Röntgendaten in Pink und optische Daten von CFHT in Blau. Dieses Zwerggalaxienpaar scheint sich in den späten Stadien einer Verschmelzung zu befinden und weist lange Schweife auf, die durch Gezeiteneffekte der Kollision verursacht werden. Die Autoren der neuen Studie nannten es Mirabilis, nachdem es vom Aussterben bedroht ist[{“ attribute=““>species of hummingbird known for their exceptionally long tails. Only one name was chosen because the merger of two galaxies into one is almost complete. The two Chandra sources show X-rays from material around the black holes in each galaxy.
The other pair was discovered in Abell 1758S, a galaxy cluster about 3.2 billion light-years away. The composite image from Chandra and CFHT is on the right, using the same colors as for Mirabilis. The researchers nicknamed the merging dwarf galaxies “Elstir” and “Vinteuil,” after fictional artists from Marcel Proust’s “In Search of Lost Time”. Vinteuil is the galaxy on the top and Elstir is the galaxy on the bottom. Both have Chandra sources associated with them, again from X-rays from material around the black holes in each galaxy. The researchers think these two have been caught in the early stages of a merger, causing a bridge of stars and gas to connect the two colliding galaxies from their gravitational interaction.
The details of merging black holes and dwarf galaxies may provide insight to our Milky Way’s own past. Scientists think nearly all galaxies began as dwarf or other types of small galaxies and grew over billions of years through mergers. Follow-up observations of these two systems will allow astronomers to study processes that are crucial for understanding galaxies and their black holes in the earliest stages of the Universe.
Ein Artikel, der diese Ergebnisse beschreibt, wurde in einer kürzlich erschienenen Ausgabe von veröffentlicht Die[{“ attribute=““>Astrophysical Journal.
Reference: “Two Candidates for Dual AGN in Dwarf-Dwarf Galaxy Mergers” by Marko Mićić, Olivia J. Holmes, Brenna N. Wells and Jimmy A. Irwin, 22 February 2023, The Astrophysical Journal.
DOI: 10.3847/1538-4357/aca1bb
The authors of the study are Marko Micic, Olivia Holmes, Brenna Wells, and Jimmy Irwin, all from the University of Alabama at Tuscaloosa.
NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.