L. Scelsi
University of Palermo
21 Papers
555 Citations
L. Scelsi is an academic researcher from University of Palermo. The author has contributed to research in topics: Stars & T Tauri star. The author has an hindex of 16, co-authored 21 publications. Previous affiliations of L. Scelsi include INAF.
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Papers
The XMM-Newton extended survey of the Taurus molecular cloud (XEST)
Manuel Güdel,Kevin Briggs,K. Arzner,Marc Audard,Jerome Bouvier,E. D. Feigelson,E. Franciosini,Adrian Glauser,Nicolas Grosso,Giuseppina Micela,J. L. Monin,Thierry Montmerle,Deborah Padgett,Francesco Palla,Ignazio Pillitteri,Luisa Rebull,L. Scelsi,Bruno Silva,Stephen L. Skinner,Beate Stelzer,A. Telleschi +20 more
TL;DR: The XMM-Newton Extended Survey of the Taurus Molecular Cloud (EST) presented in this article surveys the most populated =5 square degrees of TMC, using the XMMNewton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association.
The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)
Manuel Guedel,Kevin Briggs,K. Arzner,Marc Audard,Jerome Bouvier,E. D. Feigelson,E. Franciosini,Adrian Glauser,N. Grosso,Giuseppina Micela,J. L. Monin,T. Montmerle,Deborah Padgett,Francesco Palla,Ignazio Pillitteri,Luisa Rebull,L. Scelsi,Bruno Silva,Stephen L. Skinner,Beate Stelzer,A. Telleschi +20 more
TL;DR: The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) as discussed by the authors surveys the most populated 5 square degrees of Taurus star formation region, using the XMMNewton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association.
High Resolution X-ray Spectroscopy of T Tauri Stars in the Taurus-Auriga Complex
TL;DR: In this paper, high-resolution X-ray spectroscopy of nine pre-main sequence stars in order to test the proposed spectroscopic differences between accreting and non-accreting pre- main sequence stars was presented.
The XMM-Newton Optical Monitor Survey of the Taurus Molecular Cloud
Marc Audard,Marc Audard,Kevin Briggs,Nicolas Grosso,Manuel Guedel,L. Scelsi,Jerome Bouvier,A. Telleschi +7 more
TL;DR: In this paper, the optical monitor (OM) on-board XMM-Newton obtained optical/ultraviolet data for the XMMNewton Extended Survey of the Taurus Molecular Cloud (XEST), simultaneously with the X-ray detectors.
The XMM-Newton Optical Monitor survey of the Taurus molecular cloud
TL;DR: In this article, the optical monitor (OM) on-board XMM-Newton obtained optical/ultraviolet data for the XMMNewton Extended Survey of the Taurus Molecular Cloud (XEST), simultaneously with the X-ray detectors.