activity
20022010
most citedX-ray properties of protostars in the Orion Nebula

85 citations · 557 across the 15 of their papers we have counts for

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Showing 2006Show all

6 papers · 1 filter

astro-ph200676 cited

Unveiling the Cygnus OB2 stellar population with Chandra

J. F. Albacete Colombo, E. Flaccomio, G. Micela +2

The aim of this work is to identify the so far unknown low mass stellar population of the ~2Myr old Cygnus OB2 region, and to investigate the X-ray and near-IR stellar properties o…

astro-ph200683 cited

A statistical analysis of X-ray variability in pre-main sequence objects of the Taurus Molecular Cloud

B. Stelzer, E. Flaccomio, K. Briggs +5

This work is part of a systematic X-ray survey of the Taurus star forming complex with XMM-Newton. We study the time series of all X-ray sources associated with Taurus members, to…

astro-ph200612 cited

XMM-Newton survey of two Upper Scorpius regions

C. Argiroffi, F. Favata, E. Flaccomio +4

We study X-ray emission from young stars by analyzing deep XMM-Newton observations of two regions of the Upper Scorpius association, having an age of 5 Myr. Based on near infrared…

astro-ph200659 cited

A Simultaneous Optical and X-ray Variability Study of the Orion Nebula Cluster. I. Incidence of Time-Correlated X-ray/Optical Variations

Keivan G. Stassun, M. van den Berg, Eric Feigelson +1

We present a database of time-series photometry of the Orion Nebula Cluster obtained with two ground-based telescopes at different longitudes to provide simultaneous coverag…

astro-ph200677 cited

ACIS-I observations of NGC2264. Membership and X-ray properties of PMS stars

E. Flaccomio, G. Micela, S. Sciortino

We analyze a deep, 100 ksec long, Chandra ACIS observation of NGC2264. We detect 420 sources, 85% of which are associated with known optical and NIR counterparts. More than 90% of…

astro-ph200634 cited

Chandra X-Ray Observations of Young Clusters. III. NGC 2264 and the Orion Flanking Fields

L. M. Rebull, J. R. Stauffer, S. V. Ramirez +5

Chandra observations of solar-like pre-main sequence (PMS) stars in the Orion Flanking Fields (age ~1 Myr) and NGC 2264 (~3 Myr) are compared with the results of the COUP survey of…