E
Emanuele Tognelli
Researcher at University of Pisa
Publications - 69
Citations - 1827
Emanuele Tognelli is an academic researcher from University of Pisa. The author has contributed to research in topics: Stars & Open cluster. The author has an hindex of 22, co-authored 67 publications receiving 1628 citations. Previous affiliations of Emanuele Tognelli include INAF & Istituto Nazionale di Fisica Nucleare.
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Journal ArticleDOI
The Pisa pre-main sequence tracks and isochrones - A database covering a wide range of Z, Y, mass, and age values
TL;DR: In this article, an evolutionary pre-main sequence (pre-MS) model and isochrones for a fine grid of mass, age, metallicity, and helium values are presented.
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Instantaneous Starburst of the Massive Clusters Westerlund 1 and NGC 3603 YC
Natalia Kudryavtseva,Natalia Kudryavtseva,Wolfgang Brandner,Mario Gennaro,Boyke Rochau,Andrea Stolte,Morten Andersen,Nicola Da Rio,Thomas Henning,Emanuele Tognelli,David W. Hogg,Simon Clark,Rens Waters +12 more
TL;DR: In this article, a method to determine the age spread of resolved stellar populations in a starburst cluster is presented. But the method relies on a two-step process, in which kinematic members of the cluster are identified based on multi-epoch astrometric monitoring and a Bayesian analysis is carried out, comparing the observed photometric sequence of cluster members with sets of theoretical isochrones.
Journal ArticleDOI
Instantaneous starburst of the massive clusters Westerlund 1 and NGC 3603 YC
Natalia Kudryavtseva,Wolfgang Brandner,Mario Gennaro,Boyke Rochau,Andrea Stolte,Morten Andersen,Nicola Da Rio,Thomas Henning,Emanuele Tognelli,David W. Hogg,Simon Clark,Rens Water +11 more
TL;DR: In this article, a method to determine the age spread of resolved stellar populations in a starburst cluster is presented. But the method relies on a two-step process, in which kinematic members of the cluster are identified based on multi-epoch astrometric monitoring and a Bayesian analysis is carried out, comparing the observed photometric sequence of cluster members with sets of theoretical isochrones.
Journal ArticleDOI
On the RR Lyrae Stars in Globulars. IV. ω Centauri Optical UBVRI Photometry
V. F. Braga,V. F. Braga,V. F. Braga,Peter B. Stetson,Giuseppe Bono,Giuseppe Bono,Massimo Dall'Ora,I. Ferraro,Giuliana Fiorentino,L. M. Freyhammer,G. Iannicola,M. Marengo,Jillian R. Neeley,Elena Valenti,R. Buonanno,R. Buonanno,Annalisa Calamida,Marco Castellani,R. da Silva,R. da Silva,Scilla Degl'Innocenti,A. Di Cecco,M. Fabrizio,M. Fabrizio,Wendy L. Freedman,G. Giuffrida,G. Giuffrida,J. Lub,Barry F. Madore,Marcella Marconi,S. Marinoni,S. Marinoni,Noriyuki Matsunaga,M. Monelli,S. E. Persson,A. M. Piersimoni,Adriano Pietrinferni,P. Prada-Moroni,L. Pulone,R. F. Stellingwerf,Emanuele Tognelli,Alistair R. Walker +41 more
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Testing pre-main-sequence models: the power of a Bayesian approach
TL;DR: In this paper, a Bayesian method was developed for testing the present generation of pre-main-sequence (PMS) models against observations of PMS stars with dynamically determined masses.