activity
20032009
most citedUV excess measures of accretion onto young very low-mass stars and brown dwarfs

399 citations · 1.1k across the 8 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2009162 cited

Variable Sodium Absorption in a Low-Extinction Type Ia Supernova

Joshua D. Simon, Avishay Gal-Yam, Orly Gnat +18

Recent observations have revealed that some Type Ia supernovae exhibit narrow, time-variable Na I D absorption features. The origin of the absorbing material is controversial, but…

astro-ph.SR200995 cited

Measuring tiny mass accretion rates onto young brown dwarfs

Gregory J. Herczeg, Kelle L. Cruz, Lynne A. Hillenbrand

We present low-resolution Keck I/LRIS spectra spanning from 3200-9000 A of nine young brown dwarfs and three low-mass stars in the TW Hya Association and in Upper Sco. The optical…

astro-ph200855 cited

The TEXES Survey For H2 Emission From Protoplanetary Disks

M. A. Bitner, M. J. Richter, J. H. Lacy +9

We report the results of a search for pure rotational molecular hydrogen emission from the circumstellar environments of young stellar objects with disks using the Texas Echelon Cr…

astro-ph2008399 cited

UV excess measures of accretion onto young very low-mass stars and brown dwarfs

Gregory J. Herczeg, Lynne A. Hillenbrand

Low-resolution spectra from 3000-9000 AA of young low-mass stars and brown dwarfs were obtained with LRIS on Keck I. The excess UV and optical emission arising in the Balmer and Pa…

astro-ph200770 cited

High-resolution Spectroscopy of [Ne II] Emission from TW Hya

Gregory J. Herczeg, Joan Najita, Lynne A. Hillenbrand +1

We present high-resolution echelle spectra of [Ne II] 12.81 micron emission from the classical T Tauri star (CTTS) TW Hya obtained with MICHELLE on Gemini North. The line is center…

astro-ph200657 cited

How Hot is the Wind from TW Hydrae?

C. M. Johns-Krull, G. J. Herczeg

It has recently been suggested that the winds from Classical T Tauri stars in general, and the wind from TW Hya in particular, reaches temperatures of at least 300,000 K while main…