411 citations · 7.5k across the 155 of their papers we have counts for
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Pre-main sequence stars with disks in the Eagle Nebula observed in scattered light
M. G. Guarcello, F. Damiani, G. Micela +3
NGC6611 and its parental cloud, the Eagle Nebula (M16), are well-studied star-forming regions, thanks to their large content of both OB stars and stars with disks and the observed…
Results from DROXO. III. Observation, source list and X-ray properties of sources detected in the "Deep Rho Ophiuchi XMM-Newton Observation"
I. Pillitteri, S. Sciortino, E. Flaccomio +8
X-rays from very young stars are powerful probes to investigate the mechanisms at work in the very first stages of the star formation and the origin of X-ray emission in very young…
The New Hard X-ray Mission
G. Tagliaferri, G. Pareschi, A. Argan +12
The Italian New Hard X-ray Mission (NHXM) has been designed to provide a real breakthrough on a number of hot astrophysical issues that includes: black holes census, the physics of…
A detailed study of the rise phase of a long duration X-ray flare in the young star TWA 11B
J. Lopez-Santiago, I. Crespo-Chacon, G. Micela +1
We analyzed a long duration flare observed in a serendipitous XMM-Newton detection of the M star CD-39 7717B (TWA 11B), member of the young stellar association TW Hya (~ 8 Myr). On…
A scenario of planet erosion by coronal radiation
J. Sanz-Forcada, I. Ribas, G. Micela +4
Context: According to theory, high-energy emission from the coronae of cool stars can severely erode the atmospheres of orbiting planets. No observational tests of the long term ef…