April 2024

The position of the three stellar black holes discovered so far in the Milky Way, represented in projection, thanks to the Gaia mission.

An article published in the journal “Astronomy and Astrophysics Letters” reports the identification of a stellar black hole with a mass estimated to be approximately 33 times the Sun’s that was cataloged as Gaia BH3. A team of researchers used data collected by ESA’s Gaia space probe to find this black hole in the Milky Way’s halo, less than two thousand light-years from Earth. Its mass is remarkable for a stellar black hole and it has a companion, a very ancient star, as its age is estimated to be around 11 billion years.

Artist's impression of the GRB221009A gamma-ray burst with relativistic jets coming from the black hole at the center (Image courtesy Aaron M. Geller / Northwestern / CIERA / IT Research Computing and Data Services)

An article published in the journal “Nature Astronomy” reports a study on the gamma-ray burst cataloged as GRB221009A, the brightest ever detected, which confirms that it was caused by the collapse of a massive star, which subsequently exploded in a supernova. A team of researchers led by Northwestern University used data collected with the James Webb Space Telescope and the ALMA radio telescope to obtain the information needed to support their conclusions. The mystery remains of the absence of traces of the generation of heavy elements such as platinum and gold, which they thought could be associated with supernovae that lead to very powerful gamma-ray bursts.

The nebula NGC 6164/6165 surrounding the system HD 148937 as seen by the VLT Survey Telescope (Image ESO/VPHAS+ team. Acknowledgment: CASU)

An article published in the journal “Science” reports a study on the HD 148937 system, a binary system surrounded by a double nebula known as NGC 6164/6165. A team of researchers used the PIONIER and GRAVITY instruments mounted on ESO’s VLT Interferometer (VLTI) in Chile and archival data from the FEROS instrument at the La Silla Observatory, also an ESO’s telescope in Chile, to collect the data necessary to conclude that it was originally at least a triple system and at some point two of the stars merged. It was a violent event that created the cloud of materials around the system.

The Soyuz MS-24 spacecraft surrounded by the support crew (Image NASA TV)

A little while ago, cosmonauts Oleg Novitsky and Marina Vasilevskaya and astronaut Loral O’Hara returned to Earth on the Soyuz MS-24 spacecraft, which landed in Kazakhstan. Novitsky completed a one-year mission on the International Space Station, Vasilevskaya was a visitor who stayed on the Station for a few days while O’Hara spent a bit more than 6 months on the Station.

The M82 galaxy in Hubble's view on the left and the area of very intense star formation seen by Webb on the right

An article submitted for publication in “The Astrophysical Journal” reports a study of the exceptional rate of star formation in the M82 galaxy. A team of researchers led by Alberto Bolatto of the University of Maryland, College Park, used the James Webb Space Telescope to map powerful galactic winds that expel vast amounts of gas caused by star formation and supernova explosions.

The NIRCam instrument is the one used in particular to trace the origin of that activity back to dense star clusters in the galactic disk. This new study of M82 offers advances in understanding star formation and how this activity is affecting the galaxy.