Multifrequency Behaviour of High Energy Cosmic Sources
After the long interruption of the Frascati Workshops series due to the Covid-19 Pandemic, we are finally able to restart this historic series in complete safety. This is the fourteenth edition of the series of Frascati Workshops on "Multifrequency Behaviour of High Energy Cosmic Sources" which is undoubtedly a largely accepted biennial meeting in which an updated experimental and theoretical panorama will be depicted. This edition comes at the 39th anniversary of the first historical "multifrequency" workshop about "Multifrequency Behaviour of Galactic Accreting Sources", held in Vulcano (Archipelago of the Eolian Islands) in September 1984.
This surely renders the Frascati Workshop Series the oldest among the many devoted to "Multifrequency Studies of Cosmic Sources".
The study of the physics governing the cosmic sources will be the main goal of the workshop considering also the recent detection of gravitational waves from the merging of collapsed objects. A session devoted to the ongoing and next generation ground- and space-based experiments will give the actual prospects for the first decades of this millennium.
We deliberately do not want to change the workshop name from "Multifrequency Behavior of High Energy Cosmic Sources" to "Multimessenger Behavior of High Energy Cosmic Sources" in order to preserve the name of our historical workshop series.
• The following items will be reviewed:Cosmology: Cosmic Background, Clusters of Galaxies
• Extragalactic Sources: Active Galaxies, Normal Galaxies
• Gamma-Rays Burst: Experiments versus Theories
• Galactic Sources: Pre-Main-Sequence and Main-Sequence Stars, Cataclysmic Variables and Novae, Supernovae and SNRs, X-Ray Binary Systems, Pulsars, Black Holes, Gamma-Ray Sources,Nucleosynthesis.
• Gravitationl waves: Theory Vs Experiments.
• Science from large area multiwavelength surveys and deep-exposure pointings.
• The Astrophysics with the Ongoing and Future Experiments: Space-Based Experiments,Ground-Based Experiments.
Participation in the workshop is by invitation only.
All participants are kindly invited to attend the whole workshop.
The workshop will include several 30-min talks to introduce the current problems, and typically 20-min talks giving new experimental and theoretical results.
A series of 15-min talks will be devoted to ongoing and next generation experiments.
This is the thirteenth edition of the series of Frascati Workshops on "Multifrequency Behaviour of High Energy Cosmic Sources" which is undoubtedly a largely accepted biennial meeting in which an updated experimental and theoretical panorama will be depicted. This edition comes at the 35th anniversary of the first historical "multifrequency" workshop about "Multifrequency Behaviour of Galactic Accreting Sources", held in Vulcano in September 1984. This surely renders the Frascati Workshop Series the oldest among the many devoted to "Multifrequency Studies of Cosmic Sources". The study of the physics governing the cosmic sources will be the main goal of the workshop. A session devoted to the ongoing and next generation ground- and space-based experiments will give the actual prospects for the first decades of this millennium.
The following items will be reviewed:
• Cosmology
• Gravitational Waves
• Star Formation
• Astrophysics of High Energy Galactic and Extragalactic Cosmic Sources:
• Jet Sources and Gamma-Ray Bursts
• The Astrophysics with the Ongoing and Future Experiments: Space-based Experiments, Ground-Based Experiments
The workshop will include few 30-minute general review talks to introduce the current problems, and typically 20-minute talks discussing new experimental and theoretical results. A series of 20-minute talks will discuss the ongoing and planned ground- and space-based experiments.
The cadence of the workshop is biennial.
The participation will be only by invitation.
All participants are kindly invited to attend the whole workshop.
This is the twelfth edition of the series of Frascati Workshops on "Multifrequency Behaviour of High Energy Cosmic Sources" which is undoubtedly a largely accepted biennial meeting in which an updated experimental and theoretical panorama will be depicted. This edition comes at the 33rd anniversary of the first historical "multifrequency" workshop about "Multifrequency Behaviour of GalacticAccreting Sources", held in Vulcano in September 1984. This surely renders the Frascati Workshop Series the oldest among the many devoted to "Multifrequency Studies of Cosmic Sources". The study of the physics governing the cosmic sources will be the main goal of the workshop. A session devoted to the ongoing and next generation ground- and space-based experiments will give the actual prospects for the first decades of this millennium.
The following items will be reviewed:
- Cosmology: Cosmic Background, Clusters of Galaxies
- Extragalactic Sources: Active Galaxies, Normal Galaxies
- Gamma-Rays Burst: Experiments versus Theories
- Galactic Sources: Pre-Main-Sequence and Main-Sequence Stars, Cataclysmic Variables and Novae, Supernovae and SNRs, X-Ray Binary Systems, Pulsars, Black Holes, Gamma-Ray Sources,Nucleosynthesis.
- The Astrophysics with the Ongoing and Future Experiments: Space-Based Experiments,Ground-Based Experiments.
The workshop will include few 30-minute general review talks to introduce the current problems, and typically 20-minute talks discussing new experimental and theoretical results. A series of 20-minute talks will discuss the ongoing and planned ground- and space-based experiments.
The cadence of the workshop is biennial.
The participation will be only by invitation.
All participants are kindly invited to attend the whole workshop.
However, to keep alive the workshop it was decided that all presentations should be compulsorily given to the LOC, so that they can be inserted into the web page of the workshop. These presentations will form the basis for writing the papers to be published in the proceedings of the Frascati Workshop 2017 in electronic form by the Proceedings of Science (PoS-SISSA), after a peer referee process, and they will be freely available at once in the NASA-ADS.
The editors of the proceedings will be Franco Giovannelli and Lola Sabau-Graziati.
The study of the physics governing the cosmic sources was the main goal of the workshop. A session devoted to the ongoing and next generation ground- and space-based experiments gave the actual prospects for the first decades of this millennium. The following items have been reviewed:
Cosmology: Cosmic Background, Clusters of Galaxies
Extragalactic Sources: Active Galaxies, Normal Galaxies
Gamma-Rays Burst: Experiments versus Theories
Galactic Sources: Pre-Main-Sequence and Main-Sequence Stars, Cataclysmic Variables and Novae, Supernovae and SNRs, X-Ray Binary Systems, Pulsars, Black Holes, Gamma-Ray Sources,Nucleosynthesis.
The Astrophysics with the Ongoing and Future Experiments: Space-Based Experiments, Ground-Based Experiments.
The workshop included a few 30-minute general review talks to introduce the current problems, and typically 20-minute talks discussing new experimental and theoretical results. A series of 20-minute talks discussed the ongoing and planned ground- and space-based experiments.
The cadence of the workshop is biennial. The participation is only by invitation.