activity
20032026
most citedResolved Images of Large Cavities in Protoplanetary Transition Disks

650 citations · 7.8k across the 136 of their papers we have counts for

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Showing 2024Show all

7 papers · 1 filter

astro-ph.EP2024★ 34 cited

A giant planet transiting a 3-Myr protostar with a misaligned disk

Madyson G. Barber, Andrew W. Mann, Andrew Vanderburg +35

Astronomers have found more than a dozen planets transiting 10-40 million year old stars, but even younger transiting planets have remained elusive. A possible reason for the lack…

astro-ph.SR2024

A Model of the C IV 1548, 1550 Doublet Line in T Tauri Stars

Thanawuth Thanathibodee, Connor Robinson, Nuria Calvet +7

The C IV doublet in the UV has long been associated with accretion in T Tauri stars. However, it is still unclear where and how the lines are formed. Here, we present a new C IV li…

astro-ph.SR2024

Evidence for Dust Depletion in a Misaligned Protoplanetary Disk with JWST

C. C. Espaillat, T. Thanathibodee, Z. Zhu +12

Here we report the detection of dust depletion in a misaligned inner disk around UX Tau A using JWST MIRI spectra. Mid-infrared (MIR) continuum "seesaw" variability was detected in…

astro-ph.SR2024

A Multi-wavelength, Multi-epoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. III. Optical Spectra

John Wendeborn, Catherine C. Espaillat, Thanawuth Thanathibodee +20

Classical T Tauri Stars (CTTSs) are highly variable stars that possess gas- and dust-rich disks from which planets form. Much of their variability is driven by mass accretion from…

astro-ph.SR2024

A Multi-wavelength, Multi-epoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. II. Photometric Light Curves

John Wendeborn, Catherine C. Espaillat, Thanawuth Thanathibodee +8

Classical T Tauri Stars (CTTSs) are young, low-mass stars which accrete material from their surrounding protoplanetary disk. To better understand accretion variability, we conducte…

astro-ph.SR2024★ 1 cited

A Multi-wavelength, Multi-epoch Monitoring Campaign of Accretion Variability in T Tauri Stars from the ODYSSEUS Survey. I. HST FUV and NUV Spectra

John Wendeborn, Catherine C. Espaillat, Sophia Lopez +17

The Classical T Tauri Star (CTTS) stage is a critical phase of the star and planet formation process. In an effort to better understand the mass accretion process, which can dictat…