Personal tools
Log in

Skip to content. | Skip to navigation

INAF

Istituto italiano di astrofisica - national institute for astrophisics

Ciao
You are here: Home INAF News Carina Nebula, INAF identifies new star formations

Carina Nebula, INAF identifies new star formations

The Gaia-ESO Survey: Global properties of clusters Trumpler 14 and 16 in the Carina nebula study conducted by Francesco Damiani from INAF of Palermo, involving a number of researchers from the INAF observatories of Arcetri, Bologna, Catania, Padua and Palermo, has been recently published in Astronomy & Astrophysics.

The Gaia-ESO Survey: Global properties of clusters Trumpler 14 and 16 in the Carina nebula study conducted by Francesco Damiani from INAF of Palermo, involving a number of researchers from the INAF observatories of Arcetri, Bologna, Catania, Padua and Palermo, has been recently published in Astronomy & Astrophysics. The study carried out a spectroscopic analysis of a sample of 1085 stars belonging to the Carina region, and in particular to clusters Trumpler 14 and 16.

Stars form in huge clouds of more or less dense gas, which, under the effect of gravity, contracts and form star clusters or associations: there are particularly productive star formation regions that can generate tens of thousands of small stars and a few massive stars.

The Carina Nebula is one of the most interesting regions of massive star formation in the Milky Way, after Cygnus Ob2, the closest to us. In the Nebula, a rich population of stars has formed, which currently includes 14,000 stars already identified, including some massive stars.

The study conducted by Francesco Damiani presents the first spectroscopic analysis of a sample of 1085 stars belonging to Carena, and in particular those belonging to the rich star clusters Trumpler 14 and 16, by using data from the Gaia-Eso Survey. This is how 286 new members have been identified and a detailed analysis has been carried out on the nebula, the stars associated with the region and the chronology of star formation. Moreover, data related to the rotation speed of the stars studied were presented, by highlighting that stars older than 3 million years rotate more slowly than younger stars.

Source: ResearchItaly

Filed under: ,

CALVERA EXPLODED WHERE IT SHOULDN’T HAVE: A “RUNAWAY” PULSAR DEFIES THE RULES OF THE MILKY WAY

Aug 29, 2025

CALVERA EXPLODED WHERE IT SHOULDN’T HAVE: A “RUNAWAY” PULSAR DEFIES THE RULES OF THE MILKY WAY A stellar explosion, a pulsar, and a supernova remnant - that’s the story of Calvera. Positioned more than 6,500 light-years above the Galactic plane, this system is rewriting what we know about stellar evolution in our galaxy. The research originates from a team at the Italian National Institute for Astrophysics (INAF), in collaboration with the University of Palermo, and is detailed in a study published in Astronomy & Astrophysics

Lake Como Schools on Astrophysics, Cosmology and Gravitation

Jul 08, 2025

Lake Como Schools on Astrophysics, Cosmology and Gravitation It has been held at Como – Villa del Grumello, 23-27 June, the 2025 edition of the “Lake Como Schools on Astrophysics, Cosmology and Gravitation” on the theme “Dark Matter, Dark Energy and the Cosmological Tensions”

The Lucchin Schools Return

Jun 01, 2025

The Lucchin Schools Return First Edition of the New INAF PhD School Series Concludes in Asiago