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 2005Show all

8 papers · 1 filter

astro-ph2005

X-ray emission of brown dwarfs: Towards constraining the dependence on age, luminosity, and temperature

B. Stelzer, G. Micela, E. Flaccomio +7

Three brown dwarfs in different evolutionary stages have been observed with the Chandra X-ray Observatory. Combining the new observations with previous studies presented in the lit…

astro-ph2005

Stellar Activity on the Young Suns of Orion: COUP Observations of K5-7 Pre-Main Sequence Stars

S. J. Wolk, E. Flaccomio, G. Micela +4

In January 2003, the Chandra Orion Ultradeep Project (COUP) detected about 1400 young stars during a 13.2 day observation of the Orion Nebula Cluster (ONC). This paper studies a we…

astro-ph2005

Rotational modulation of X-ray emission in Orion Nebula young stars

E. Flaccomio, G. Micela, S. Sciortino +5

We investigate the spatial distribution of X-ray emitting plasma in a sample of young Orion Nebula Cluster stars by modulation of their X-ray light-curves due to stellar rotation.…

astro-ph2005

Bright X-ray flares in Orion young stars from COUP: evidence for star-disk magnetic fields?

F. Favata, E. Flaccomio, F. Reale +5

We have analyzed a number of intense X-ray flares observed in the Chandra Orion Ultradeep Project (COUP), a 13 days observation of the Orion Nebula Cluster (ONC). Analysis of the f…

astro-ph2005

X-ray emission from young brown dwarfs in the Orion Nebula Cluster

Thomas Preibisch, Mark J. McCaughrean, Nicolas Grosso +8

We use the sensitive X-ray data from the Chandra Orion Ultradeep Project (COUP) to study the X-ray properties of 34 spectroscopically-identified brown dwarfs with near-infrared spe…

astro-ph2005

X-ray emission from early-type stars in the Orion Nebula Cluster

B. Stelzer, E. Flaccomio, T. Montmerle +5

The X-ray properties of twenty ~1 Myr old O, B, and A stars of the Orion Trapezium are examined with data from the Chandra Orion Ultradeep Project (COUP). On the basis of simple th…