E. D. Feigelson
Pennsylvania State University
58 Papers
1.7K Citations
E. D. Feigelson is an academic researcher from Pennsylvania State University. The author has contributed to research in topics: Stars & T Tauri star. The author has an hindex of 30, co-authored 58 publications.
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Papers
Statistical methods for astronomical data with upper limits. II - Correlation and regression
TL;DR: In this article, survival analysis is applied to CO emission in infrared galaxies, X-ray emission in radio galaxies, H-alpha emission in cooling cluster cores, and radio emission in Seyfert galaxies.
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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.
Ten Million Degree Gas in M 17 and the Rosette Nebula: X-ray Flows in Galactic H II Regions
Leisa K. Townsley,E. D. Feigelson,T. Montmerle,Patrick S. Broos,You-Hua Chu,Gordon P. Garmire +5 more
TL;DR: In this article, the first high-spatial-resolution X-ray images of two high-mass star forming regions, the Omega Nebula (M 17) and the Rosette Nebula (NGC 2237--2246), were obtained with the Chandra Xray Observatory Advanced CCD Imaging Spectrometer (ACIS) instrument.
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A Chandra Study of Sgr A East: A Supernova Remnant Regulating The Activity Of Our Galactic Center?
Yoshitomo Maeda,Frederick K. Baganoff,E. D. Feigelson,Mark Morris,Marshall W. Bautz,W. N. Brandt,D. N. Burrows,John P. Doty,Gordon P. Garmire,S. Pravdo,George R. Ricker,Leisa K. Townsley +11 more
TL;DR: In this article, the X-ray emission from the shell-like, non-thermal radio source Sgr A East located in the inner few parsecs of the Galaxy based on observations made with the ACIS detector on board Chandra.
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