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Quaternary Geochronology, ISSN 1871-1014, 09/2016, Volume 36, pp. 67 - 75
The Middle Pleistocene archaeological site of Guado San Nicola was discovered in 2005 in a fossil fluvial terrace of the Volturno River, close to the village... 
Ar | Italy | Ar dating | Middle Palaeolithic transition | ESR/U-series | Levallois technologies | Earth Sciences | Nuclear Experiment | Sciences of the Universe | Humanities and Social Sciences | Paleontology | Physics | Archaeology and Prehistory
Journal Article
QUATERNARY GEOCHRONOLOGY, ISSN 1871-1014, 09/2016, Volume 36, pp. 67 - 75
The Middle Pleistocene archaeological site of Guado San Nicola was discovered in 2005 in a fossil fluvial terrace of the Volturno River, close to the village... 
Ar-40/Ar-39 dating | ESR/U-series | TUFF | U-UPTAKE | GEOCHRONOLOGY | SANIDINE | GEOGRAPHY, PHYSICAL | GEOSCIENCES, MULTIDISCIPLINARY | EVOLUTION | TOOTH ENAMEL | Middle Palaeolithic transition | Levallois technologies | Italy | VOLCANO ROMAN REGION | STANDARD
Journal Article
Quaternary Geochronology, ISSN 1871-1014, 09/2016, Volume 36, pp. 67 - 75
The Middle Pleistocene archaeological site of Guado San Nicola was discovered in 2005 in a fossil fluvial terrace of the Volturno River, close to the village... 
Middle Palaeolithic transition | 40Ar/39Ar dating | ESR/U-series | Levallois technologies | Italy
Journal Article
Quaternary International, ISSN 1040-6182, 09/2017, Volume 450, pp. 5 - 11
In the last decades, debates on the origin, timing and spread of the Levallois method and its relation with the end of the Acheulean and transition to the... 
Italian Peninsula | Lower Palaeolithic | Guado San Nicola | Isernia La Pineta | Levallois | Acheulean
Journal Article
QUATERNARY INTERNATIONAL, ISSN 1040-6182, 09/2017, Volume 450, pp. 5 - 11
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 10/2009, Volume 505, Issue 1, pp. 405 - 415
Context. The majority of stars form in clusters. Therefore a comprehensive view of star formation requires understanding the initial conditions for cluster... 
MILLIMETER | CORES | MOLECULAR CLOUDS | STAR-FORMATION | MAIN CLOUD | stars: formation | INTERSTELLAR EXTINCTION | DUST | CLUSTERS | catalogs | ASTRONOMY & ASTROPHYSICS | ISM: clouds | MILKY-WAY | NGC-2264 | Physics - Astrophysics of Galaxies
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2013, Volume 553, pp. A119 - 18
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2016, Volume 455, Issue 1, pp. 806 - 819
Much of the dense gas in molecular clouds has a filamentary structure but the detailed structure and evolution of this gas is poorly known. We have observed 54... 
Molecules | ISM | Clouds | Massive | Stars | Submillimetre | Formation | MILLIMETER | submillimetre: ISM | AMMONIA | DEUTERIUM FRACTIONATION | MASSIVE-STAR-FORMATION | DYNAMICAL COLLAPSE | CLUMPS | stars: formation | ISM: molecules | ASTRONOMY & ASTROPHYSICS | DENSE CORES | stars: massive | ISM: clouds | LINE-PROFILES | PROBE | EVOLUTIONARY TRACER | Star & galaxy formation | Dispersion | Astronomy | Kinematics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2017, Volume 470, Issue 4, pp. 3882 - 3923
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 448, Issue 3, pp. 2344 - 2361
Journal Article