January 2018

The Tarantula Nebula (Image X-ray: NASA/CXC/PSU/L.Townsley et al.; Optical: NASA/STScI; Infrared: NASA/JPL/PSU/L.Townsley et al.)

An article published in the journal “Science” describes the really out-of-the-ordinary amount of massive stars discovered in the Tarantula Nebula, a region of the Great Magellanic Cloud, one of the Milky Way’s satellite dwarfs galaxies. A team of researchers participating in the VLT-FLAMES Tarantula Survey (VFTS) used ESO’s Very Large Telescope to observe nearly 1,000 massive stars in that region concluding that there’s a much higher amount than expected by the models with various important astronomical implications.

The galaxy UGC 6093 (Image ESA/Hubble & NASA)

A photo of the galaxy UGC 6093 taken by the Hubble Space Telescope shows some of its interesting features. It’s a barred spiral galaxy, it has an active galactic nucleus powered by a supermassive black hole at its center and acts like a megamaser, which is an astronomical maser that emits microwaves with an intensity about 100 million times greater than that of the astronomical masers found in galaxies such as the Milky Way.

KIC 8462852 at infrareds and ultraviolets (Image: IPAC/NASA for infrareds, STScI (NASA) for ultraviolets)

An article published in “The Astrophysical Journal Letters” describes the results of new observations of the star KIC 8462852, commonly known as Tabby’s star or sometimes Boyajian’s star. A team of astronomers led by Tabetha S. Boyajian, the astronomer who in 2015 realized that its brightness was changing rapidly, dimming up to 20% within a few days, conducted a research possible thanks to a funding obtained through a campaign on Kickstarter. The conclusions confirm the theory of dust that obscures the star, in particular at certain frequencies.

Artist's concept of the TRAPPIST-1 system (Image NASA/JPL-Caltech)

An article published in the journal “Proceedings of the National Academy of Sciences” describes a research that tries to provide an estimate of the possibilities for the 7 planets of the ultra-cool dwarf star TRAPPIST-1 to maintain an atmosphere. A team of researchers created simulations that took into account the characteristics of TRAPPIST-1’s stellar wind and the possible speed at which the planets’ atmosphere would be torn away from them. The conclusion is that the two outermost planets could maintain an atmosphere for billions of years.