0000000000530459

AUTHOR

G. Sacco

showing 4 related works from this author

The Gaia-ESO Public Spectroscopic Survey

2012

The Gaia-ESO Public Spectroscopic Survey has begun and will obtain high quality spectroscopy of some 100000 Milky Way stars, in the field and in open clusters, down to magnitude 19, systematically covering all the major components of the Milky Way. This survey will provide the first homogeneous overview of the distributions of kinematics and chemical element abundances in the Galaxy. The motivation, organisation and implementation of the Gaia-ESO Survey are described, emphasising the complementarity with the ESA Gaia mission. Spectra from the very first observing run of the survey are presented.

spectroscopy stars kinematics abundancesSettore FIS/05 - Astronomia E AstrofisicaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Galaxy Astrophysics
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The close classical T Tauri binary V4046 Sgr: Complex magnetic fields & distributed mass accretion

2011

We report here the first results of a multi-wavelength campaign focussing on magnetospheric accretion processes within the close binary system V4046 Sgr, hosting two partly-convective classical T Tauri stars of masses ~0.9 Msun and age ~12 Myr. In this paper, we present time-resolved spectropolarimetric observations collected in 2009 September with ESPaDOnS at the Canada-France-Hawaii Telescope (CFHT) and covering a full span of 7d or ~2.5 orbital/rotational cycles of V4046 Sgr. Small circularly polarised Zeeman signatures are detected in the photospheric absorption lines but not in the accretion-powered emission lines of V4046 Sgr, thereby demonstrating that both system components host lar…

stars: formation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]stars: individual: V4046 SgrAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsstars: imagingtechniques: polarimetricSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar Astrophysicsstars: rotation[SDU]Sciences of the Universe [physics]stars: magnetic fieldsAstrophysics::Solar and Stellar Astrophysicstechniques: polarimetric stars: formation stars: imaging stars: individual: V4046 Sgr stars: magnetic fields stars: rotationAstrophysics::Earth and Planetary AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics
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Italian cancer figures, report 2014: Prevalence and cure of cancer in Italy

2015

This Report intends to estimate the total number of people still alive in 2010 after cancer diagnosis in Italy, regardless of the time since diagnosis, and to project these estimates to 2015. This study is also aimed to estimate the number of already cured cancer patients, whose mortality rates have become undistinguishable from that of the general population of the same age and sex.The study took advantage of the information from the AIRTUM database, which included 29 Cancer Registries (covering 21 million people, 35% of the Italian population). A total of 1,624,533 cancer cases diagnosed between 1976 and 2009 contributed to the study. For each registry, the observed prevalence was calcula…

Aged 80 and overMaleMedicine (all)Aged; Aged 80 and over; Female; Humans; Italy; Male; Middle Aged; Neoplasms; Prevalence; Registries; Survival RateSocio-culturaleMiddle AgedSettore MED/42 - Igiene Generale E ApplicataSurvival RateItalyNeoplasms80 and overPrevalenceHumanscancer prevalence cancer incidence cancer in ItalyFemaleRegistriesAged
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The Gaia-ESO Survey: membership and initial mass function of the. Velorum cluster

2016

Understanding the properties of young open clusters, such as the Initial Mass Function (IMF), star formation history and dynamic evolution, is crucial to obtain reliable theoretical predictions of the mechanisms involved in the star formation process. We want to obtain a list, as complete as possible, of confirmed members of the young open cluster Gamma Velorum, with the aim of deriving general cluster properties such as the IMF. We used all available spectroscopic membership indicators within the Gaia-ESO public archive together with literature photometry and X-ray data and, for each method, we derived the most complete list of candidate cluster members. Then, we considered photometry, gra…

Initial mass functionStars: luminosity function mass functionStars: formationFOS: Physical sciencesTechniques: spectroscopicOpen clusters and associations: individual: γVelorum; Stars: formation; Stars: luminosity function mass function; Stars: pre-main sequence; Techniques: radial velocities; Techniques: spectroscopic; Astronomy and Astrophysics; Space and Planetary ScienceAstrophysicsStars: luminosity function01 natural sciencesstars: pre-main sequence / open clusters and associations: individual: γVelorum / stars: formation / stars: luminosity functionPhotometry (optics)stars: pre-main sequence / open clusters and associations: individual: γVelorum / stars: formation / stars: luminosity function mass function / techniques: radial velocities / techniques: spectroscopic0103 physical sciences010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Open clusters and associations: individual: γVelorumQCQBPhysics010308 nuclear & particles physicsStar formationTechniques: radial velocitieAstronomy and Astrophysicsmass function / techniques: radial velocities / techniques: spectroscopicAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesAstrophysics - Solar and Stellar AstrophysicsYoung populationmass functionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Techniques: radial velocitiesopen clusters and associations: individual: gamma VelorumStars: pre-main sequenceOpen cluster
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