175 citations · 468 across the 11 of their papers we have counts for
7 papers · 1 filter
AB Aur, a Rosetta stone for studies of planet formation (II): HS detection and sulfur budget
Pablo Rivière-Marichalar, Asunción Fuente, Gisela Esplugues +7
The sulfur abundance is poorly known in most environments. Yet, deriving the sulfur abundance is key to understanding the evolution of the chemistry from molecular clouds to planet…
An ALMA Survey of Protoplanetary Disks in Lynds 1641
Sierra L. Grant, Catherine C. Espaillat, John Wendeborn +8
We present ALMA observations of 101 protoplanetary disks within the star-forming region Lynds 1641 in the Orion Molecular Cloud A. Our observations include 1.33 mm continuum emissi…
Revealing the Star-Disk-Jet Connection in GM Aur using Multiwavelength Variability
C. C. Espaillat, E. Macias, J. Hernandez +1
Here we analyze the first simultaneous X-ray, ultraviolet, optical, infrared, and centimeter observations of a T Tauri star (TTS). We present three epochs of simultaneous Spitzer a…
Modeling the Protoplanetary Disks of Two Brown Dwarfs in the Taurus Molecular Cloud
Anneliese M. Rilinger, Catherine C. Espaillat, Enrique Macías
Measuring the properties of protoplanetary disks around brown dwarfs is central to understanding the formation of brown dwarfs and their planetary companions. We present modeling o…
Long-lived protoplanetary disks in multiple systems: the VLA view of HD 98800
Álvaro Ribas, Enrique Macías, Catherine C. Espaillat +1
The conditions and evolution of protoplanetary disks in multiple systems can be considerably different from those around single stars, which may have important consequences for pla…
Herschel PACS observations of 4-10 Myr old Classical T Tauri stars in Orion OB1
Karina Maucó, César Briceño, Nuria Calvet +12
We present \emph{Herschel} PACS observations of 8 Classical T Tauri Stars in the Myr old OB1a and the Myr old OB1b Orion sub-asscociations. Detailed modeling…
Far-infrared to millimeter data of protoplanetary disks: dust growth in the Taurus, Ophiuchus, and Chamaeleon I star-forming regions
Álvaro Ribas, Catherine C. Espaillat, Enrique Macías +7
Far-infrared and (sub)millimeter fluxes can be used to study dust in protoplanetary disks, the building blocks of planets. Here, we combine observations from the Herschel Space Obs…