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 X-ray Astronomy: towards the next 50 years!

X-ray Astronomy: towards the next 50 years!

International conference, Oct 1st to Oct 5th, 2012, Milan (Italy)

This year we celebrate the 50th anniversary of the discovery of SCO X-1, the first extrasolar X-ray source, and of the first measure of the X-ray background by Giacconi, Gursky, Paolini, and Rossi. For this occasion, the Astronomical Observatory of Brera and the Istituto di Astrofisica Spaziale e Fisica Cosmica of INAF are organizing the conference "X-ray Astronomy: towards the next 50 years!".

The conference will be held at the Museum of Science and Technology, in Milan, where Riccardo Giacconi got his first degree in Physics, from Oct 1st to Oct 5th, 2012.

The meeting aims at providing an overall review of X-ray astronomy today, focusing on the most challenging open problems and stimulating future perspectives.

Contact: loc-xastro50@brera.inaf.it

AN "IMPROBABLE" PLANETARY SYSTEM: COMPACT, COPLANAR, AND SHAPED BY A BROWN DWARF

Jun 17, 2026

AN "IMPROBABLE" PLANETARY SYSTEM: COMPACT, COPLANAR, AND SHAPED BY A BROWN DWARF An international team involving over ten institutions, with a strong participation from ESO and INAF, has characterised TOI-201 c, the transiting brown dwarf with the longest period for which mass has been measured. The study, published today in Nature, reveals a compact, coplanar system in which the presence of a massive, eccentric object redefines the stability boundaries for the inner planets

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.