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Istituto italiano di astrofisica - national institute for astrophisics

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Science with the Cherenkov Telescope Array

The updated science case for the Cherenkov Telescope Array Observatory, Science with the Cherenkov Telescope Array, became available for download in English or Spanish on the CTA website library and arXiv
Science with the Cherenkov Telescope Array

The updated science case for the Cherenkov Telescope Array Observatory, Science with the Cherenkov Telescope Array, became available for download in English or Spanish on the CTA website library and arXiv.

Science with the Cherenkov Telescope Array will be published in a special edition of International Journal of Modern Physics D in the coming weeks. The work includes more than 200 pages that introduce and elaborate on CTA’s major science themes and place CTA in the context of other major observatories.

ALMA WITNESSES STAR BIRTH BEYOND THE EDGES OF THE MILKY WAY

Apr 22, 2026

ALMA WITNESSES STAR BIRTH BEYOND THE EDGES OF THE MILKY WAY A new study, led by INAF, has mapped, for the first time, the mass distribution of newly formed cores in the Large Magellanic Cloud. Thanks to high-resolution images from ALMA, it has emerged that these cores form according to the same patterns observed in the Milky Way. The result suggests that the initial fragmentation mechanisms of gas and dust clumps, from which stars are born, are universal and independent of the galactic environment.

RR Lyrae variables as beacons to investigate the early formation of the Milky Way

Jan 26, 2026

RR Lyrae variables as beacons to investigate the early formation of the Milky Way

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