Stars

The Running Chicken with the Moon as a reference as seen from the VST

An image captured by the VLT Survey Telescope (VST) shows a cosmic formation nicknamed the Running Chicken for the shape some see in what is actually a collection of different star-forming regions. The OmegaCAM wide-field camera mounted on the VST generated a 1.5 billion-pixel image that includes never-before-seen detail in an area 25 times the size of the full Moon. The brightest region in the nebula is cataloged as IC 2948 and corresponds to what some see as the chicken’s head and others as its rear end. Towards the center of the image, at a pillar-like structure, there’s a region cataloged as IC 2944. The brightest star is actually closer and is known as Lambda Centauri.

central area of the star-forming area IC 348 seen by the James Webb Space Telescope's NIRCam instrument. Zooms in the insets show the three brown dwarfs discovered in this study.

An article published in “The Astronomical Journal” reports the discovery of three brown dwarfs in the star formation area cataloged as IC 348, part of the large Perseus Cloud. A team of researchers used the James Webb Space Telescope to study that area searching for brown dwarf candidates and identifying three with masses less than eight times Jupiter’s. The smallest of them has a mass estimated between three and four times Jupiter’s, making it the smallest known brown dwarf. Two of them show the chemical signatures of an unidentified aliphatic hydrocarbon whose presence is not predicted by any atmospheric model.

The Cassiopeia A supernova remnant

An image of the Cassiopeia A supernova remnant (NASA, ESA, CSA, STScI, Danny Milisavljevic (Purdue University), Ilse De Looze (UGent), Tea Temim (Princeton University)), or simply Cas A, captured by the James Webb Space Telescope’ NIRCam instrument shows new details of the structures present among the materials surrounding what remains of the progenitor star. In April 2023, images captured by another Webb instrument, MIRI, were published, showing different details of Cassiopeia A. The reasons why certain structures are invisible to NIRCam are also being studied.

The central area of the Milky Way as seen by the Subaru telescope. Several stars are visible in an area about 0.4 light-years across. The star S0-6 is circled in blue while the area where the supermassive black hole Sagittarius A* is located is circled in green.

An article published in the journal “Proceedings of the Japan Academy, Series B, Physical and Biological Sciences” reports a study on the star cataloged as S0-6 which indicates that it formed in another galaxy and only over time reached the center of the Milky Way. Since 2014, a team of researchers led by Shogo Nishiyama of Miyagi University of Education in Japan has been studying various stars that now orbit Sagittarius A*, or simply Sgr A*, the supermassive black hole at the center of the Milky Way.

The HH 1177 system

An article published in the journal “Nature” reports the identification of a protoplanetary disk around the very young star cataloged as HH 1177 in the Large Magellanic Cloud, one of the dwarf galaxies satellite of the Milky Way. A team of researchers used the ALMA radio telescope to observe the disk in a follow-up study after observations conducted with the MUSE instrument mounted on the VLT allowed to see jets coming from the still-forming star. This is the first detection of a circumstellar disk in another galaxy. That type of structure is also called a Keplerian disk in jargon because it obeys the same laws as planetary motion.