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Specola M. Hack

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In remote nubi di gas, le tracce delle prime stelle

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Created: Thursday, 04 May 2023 10:16

Scoperte le impronte lasciate dall’esplosione delle prime stelle dell’universo in nubi di gas risalenti a 11 miliardi di anni fa, osservate attraverso il Very Large Telescope dell’European Southern Observatory da un team internazionale di cui fanno parte ricercatrici e ricercatori dell'INAF di Trieste e dell'Università di Firenze.

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New evidence for the nature of matter from ancient galaxies in the early Universe

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Created: Wednesday, 29 March 2023 12:36

Astrophysicists in Italy have shed new light on the nature of matter from the James Webb Space Telescope (JWST) galaxy detections 13 billion years ago and novel state-of-the-art numerical simulations of the first galaxies. The study adds another piece to the puzzle of the nature of matter in the Universe.

While the commonly accepted paradigm of structure formation is based on non-relativistic matter that interacts only gravitationally, that is ‘cold’ dark matter, alternative possibilities advocated to solve small-scale problems of the standard scenario rely on the hypothesis that dark matter is made of warm particles that possess a small, non-negligible, thermal velocity, namely ‘warm’ dark matter.

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ALMA unveils the mystery about the properties of the most luminous quasar host galaxy at high redshift

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Created: Sunday, 12 February 2023 12:36

Quasars are certainly among the most mysterious objects in the Universe. And without any doubts, the quasar J0100+2802 is one of the most interesting quasars known to date, since it is the most luminous quasar with the most massive black hole at redshift z>6 (i.e. less than 900 million years from the beginning of the Universe).

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Tredici miliardi di anni sotto la luce d’antichi quasar

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Created: Wednesday, 08 March 2023 12:36

Leggendo con lo spettrografo X-Shooter del Vlt il “codice a barre” impresso nella luce di antichissimi quasar, un team di astronomi guidato dal centro australiano Astro3D – team del quale fanno parte anche Valentina D’Odorico, Guido Cupani e Manuela Bischetti dell’Inaf di Trieste – è riuscito a misurare la variazione repentina della densità di carbonio nell’universo all’epoca della reionizzazione.

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More Articles ...

  1. Dusty-wind-clear JWST Super-early Galaxies
  2. The relaxation techniques of galaxy clusters
  3. The unexplored world of MINCE: Abundances of neutron capture elements where no one is looking
  4. Pile-up in the "Bullet cluster"
  5. The interesting case of QSO J2310+1855

 

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