most citedWhy are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors?

52 citations · 119 across the 4 of their papers we have counts for

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astro-ph20084 cited

The Full Spectrum Galactic Terrarium: MHz to TeV Observations of Various Critters

Mallory S. E. Roberts, C. Brogan, S. Ransom +13

Multi-wavelength studies at radio, infrared, optical, X-ray, and TeV wavelengths have discovered probable counterparts to many Galactic sources of GeV emission detected by EGRET. T…

astro-ph200849 cited

Reflected light from 3D exoplanetary atmospheres and simulation of HD 209458b

Ben Hood, Kenneth Wood, Sara Seager +1

We present radiation transfer models that demonstrate that reflected light levels from three dimensional (3D) exoplanetary atmospheres can be more than 50% lower than those predict…

astro-ph200814 cited

IRAS04325+2402C: A very low mass object with an edge-on disk

Alexander Scholz, Ray Jayawardhana, Kenneth Wood +3

IRAS04325+2402C is a low luminosity object located near a protostar in Taurus. We present new spatially-resolved mm observations, near-infrared spectroscopy, and Spitzer photometry…

astro-ph200752 cited

Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors?

S. G. Gregory, K. Wood, M. Jardine

Accreting T Tauri stars are observed to be less luminous in X-rays than non-accretors, an effect that has been detected in various star forming regions. To explain this we have com…

astro-ph2006210 cited

Exploring brown dwarf disks: A 1.3 mm survey in Taurus

Alexander Scholz, Ray Jayawardhana, Kenneth Wood

We have carried out sensitive 1.3 mm observations of 20 young brown dwarfs in the Taurus star-forming region, representing the largest sample of young substellar objects targeted i…