Stars

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.

Filaments (in blue) that connect the galaxies (in white) of the SSA22 cluster (Image courtesy Hideki Umehata)

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An article published in the journal “Science” reports the discovery of massive gas filaments between the galaxies of a protocluster cataloged as SSA22 about 12 billion light years from Earth. A team of researchers coordinated by the RIKEN Cluster for Pioneering Research used the MUSE spectrograph mounted on the VLT in Chile and the Suprime-Cam on the Subaru telescope to map those filaments, which extend over more than 3 million light years. Follow-up observations that provided further details were conducted with the ALMA radio telescope and the Keck telescope. The filament gas can feed star formation and the growth of supermassive black holes in the protocluster. The observation of those processes can provide new information on the evolution of galaxies.

Artist's concept of tidal destruction event (Image NASA's Goddard Space Flight Center)

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An article published in “The Astrophysical Journal” reports the study of an event cataloged as ASASSN-19bt in which a supermassive black hole destroyed a star that came too close to it. A team of researchers led by Patrick Vallely and Tom Holoien discovered the start of the event thanks to the ASAS-SN network, obtained observations thanks to the NASA TESS space telescope, which was aimed at that area, and conducted follow-up observations using NASA’s Swift and ESA’s XMM-Newton space telescopes and the network of ground-based Las Cumbres Observatories.

The AFGL 4104, or Roberts 22, protoplanetary nebula (Image NASA, ESA, and R. Sahai (Jet Propulsion Laboratory))

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An article published in the journal “Monthly Notices of the Royal Astronomical Society” reports a study on the importance of the ejection of materials by stars in the last stages of their life in the formation of life forms such as those on the Earth. Professor Michael Smith and PhD student Igor Novikov of the British University of Kent performed a series of computer simulations of processes in protoplanetary nebulae obtaining results that offer important clues concerning the recycling of materials generated in stars and ejected into interstellar space.

The VISTA telescope offers new details of the Magellanic Clouds

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An article accepted for publication in the journal “Monthly Notices of the Royal Astronomical Society” reports the results of a study of the two Magellanic Clouds, satellite dwarf galaxies of the Milky Way. A team of researchers used data collected during the VISTA survey of the Magellanic Clouds system (VMC) exploiting the ability of ESO’s VISTA telescope to detect the near infrareds to show new details of the Magellanic Clouds.