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20052023
most citedObservations of Mass Loss from the Transiting Exoplanet HD 209458b

331 citations · 1.5k across the 25 of their papers we have counts for

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Showing astro-ph.SRShow all

9 papers · 1 filter

astro-ph.SR2016★ 70 cited

Cloud Atlas: Discovery of Patchy Clouds and High-amplitude Rotational Modulations In a Young, Extremely Red L-type Brown Dwarf

Ben W. P. Lew, Daniel Apai, Yifan Zhou +10

Condensate clouds fundamentally impact the atmospheric structure and spectra of exoplanets and brown dwarfs but the connections between surface gravity, cloud structure, dust in th…

astro-ph.SR2013★ 99 cited

Hot Gas Lines in T Tauri Stars

David R. Ardila, Gregory J. Herczeg, Scott G. Gregory +20

For Classical T Tauri Stars (CTTSs), the resonance lines of N V, Si IV, and C IV, as well as the He II 1640 A line, act as diagnostics of the accretion process. Here we assemble a…

astro-ph.SR2012★ 65 cited

Lyman alpha dominance of the Classical T Tauri FUV Radiation Field

Rebecca Schindhelm, Kevin France, Gregory Herczeg +6

Far-ultraviolet (FUV) radiation plays an important role in determining chemical abundances in protoplanetary disks. HI Lyman alpha is suspected to be the dominant component of the…

astro-ph.SR2012★ 110 cited

A Hubble Space Telescope Survey of H2 Emission in the Circumstellar Environments of Young Stars

Kevin France, Rebecca Schindhelm, Gregory J. Herczeg +8

The formation timescale and final architecture of exoplanetary systems are closely related to the properties of the molecular disks from which they form. Observations of the spatia…

astro-ph.SR2012★ 117 cited

A Far-ultraviolet Atlas of Low-resolution Hubble Space Telescope Spectra of T Tauri Stars

Hao Yang, Gregory J. Herczeg, Jeffrey L. Linsky +6

We present a far-ultraviolet (FUV) spectral atlas consisting of spectra of 91 pre-main sequence stars. Most stars in this sample were observed with the Space Telescope Imaging Spec…

astro-ph.SR2011★ 82 cited

NUV Excess in Slowly Accreting T Tauri Stars: Limits Imposed by Chromospheric Emission

Laura Ingleby, Nuria Calvet, Edwin Bergin +20

Young stars surrounded by disks with very low mass accretion rates are likely in the final stages of inner disk evolution and therefore particularly interesting to study. We presen…