activity
20032008
most citedThe XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

372 citations · 714 across the 9 of their papers we have counts for

collaborators

12 papers

astro-ph200887 cited

FLAMES spectroscopy of low-mass stars in the young clusters sigma Ori and lambda Ori

G. G. Sacco, E. Franciosini, S. Randich +1

Aims. We performed a detailed membership selection and studied the accretion properties of low-mass stars in the two apparently very similar young (1-10 Myr) clusters sigma Ori and…

astro-ph20071 cited

Accretion and Outflow-Related X-Rays in T Tauri Stars

M. Guedel, K. Briggs, K. Arzner +22

We report on accretion- and outflow-related X-rays from T Tauri stars, based on results from the "XMM-Newton Extended Survey of the Taurus Molecular Cloud." X-rays potentially form…

astro-ph200710 cited

X-rays from young stars - a summary of highlights from the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

M. Guedel

The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) is a survey of the nearest large star-forming region, the Taurus Molecular Cloud (TMC), making use of all instru…

astro-ph200639 cited

Lithium depleted stars in the young sigma Ori cluster

G. G. Sacco, S. Randich, E. Franciosini +2

Context: Knowledge of the age distribution of stars in young clusters and associations is crucial to constrain models of star formation. HR diagrams of different young clusters and…

astro-ph200639 cited

Spectral properties of X-ray bright variable sources in the Taurus Molecular Cloud

E. Franciosini, I. Pillitteri, B. Stelzer +7

We analyze 19 bright variable X-ray sources detected in the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), in order to characterize the variations with time of th…

astro-ph200678 cited

The first high-resolution X-ray spectrum of a Herbig Star: The case of AB Aurigae

A. Telleschi, M. Guedel, K. R. Briggs +3

We present the first high-resolution X-ray spectrum of a prototypical Herbig star (AB Aurigae), measure and interpret various spectral features, and compare our results with model…