Telescopes

Artist's concept of a planetary collision in the BD +20 307 system (Image NASA/SOFIA/Lynette Cook)

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An article published in “The Astrophysical Journal” reports a study of the BD +20 307 binary system in which the presence of dust too warm to be the equivalent of the Kuiper belt was detected, therefore they have been interpreted as the remains of a planetary collision. A team of researchers led by Maggie Thompson of the University of California at Santa Cruz used the SOFIA flying telescope to detect infrared emissions, which increased over time.

Artist's concept of MAXI J1820+070's system (Image courtesy John Paice)

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An article published in the journal “Monthly Notices of the Royal Astronomical Society” reports a study of the black hole MAXI J1820+070, part of an X-ray binary system that includes a normal star to which the black hole steals gas. A team of astronomers coordinated by the British University of Southampton used the HiPERCAM and NICER instruments to detect visible light and X-rays respectively emitted during an outburst activity in 2018. The data collected were used to create a video slowed down ten times to allow astronomers to see the fastest flares and examine the details of that activity.

Artist's concept of a quasar (Image ESO/M. Kornmesser)

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An article published in the journal “Astronomy & Astrophysics” reports an analysis of 48 quasars in the early universe to detect the outflows of materials they produce. A team of researchers led by Manuela Bischetti of the Italian National Institute of Astrophysics in Rome used the ALMA radio telescope to confirm for the first time the common existence of those outflows, which act as powerful winds inside those early galaxies heavily interfering in the formation of new stars.

Two disks that rotate in opposite directions around the supermassive black hole at the center of the galaxy NGC 1068

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An article published in the journal “The Astrophysical Journal” reports the discovery of a supermassive black hole at the center of the galaxy NGC 1068 surrounded by two gas disks that rotate in opposite directions. A team of researchers led by Caterina Maria Violette Impellizzeri of the National Radio Astronomy Observatory (NRAO) used the ALMA radio telescope to observe the center of that galaxy in sufficient detail to detect the two disks and their motions. That situation is not very stable and in the future a collision between the two rings could generate an abundant meal for the black hole. That’s a possible quick growth mechanism for supermassive black holes.

Interstellar comet 2I/Borisov (Image courtesy Gemini Observatory/Nsf/Aura)

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An article published in the journal “Nature Astronomy” reports an initial characterization of interstellar comet 2I/Borisov, initially designated as C/2019 Q4. A team of researchers used data collected using the Gemini North on the island of Mauna Kea, in Hawaii, and the William Herschel Telescope in the Canaries. The data confirm it comes from another star system, yet it has characteristics very similar to the comets of the solar system.