Discs of gas and dust around million-year-old stars are a by-product of the star formation
process and provide the raw material to form planets. Hence, their evolution and dispersal …

Flattened, rotating disks of cool dust and gas extending for tens to hundreds of astronomical
units are found around almost all low-mass stars shortly after their birth. These disks …

Terrestrial and sub-Neptune planets are expected to form in the inner (less than 10 au)
regions of protoplanetary disks. Water plays a key role in their formation,–, although it is yet …

We present new results from a significant extension of our previous high angular resolution
(0 farcs 3≈ 40 AU) submillimeter array survey of the 340 GHz (880 μm) thermal continuum …

We present a synergic study of protoplanetary disks to investigate links between inner-disk
gas molecules and the large-scale migration of solid pebbles. The sample includes 63 disks …

We present initial results from a population synthesis model aimed at determining the star
formation rate (SFR) of the Milky Way. We find that a total SFR of 0.68–1.45 M☉ yr− 1 is able …

We present a survey of optical [O i] emission at 6300 Å toward 65 T Tauri stars at the spectral
resolution of∼ 7 km s− 1. Past work identified a highly blueshifted velocity component (HVC) …

We analyze the accretion properties of 21 low-mass T Tauri stars using a data set of
contemporaneous near-UV (NUV) through optical observations obtained with the Hubble …

Since the discovery of the first extrasolar planet around a solartype star, 1 more than 900
such planets outside of our solar system have been detected by ground-and space-based …

We present an overview and first results from a M-band spectroscopic survey of planet-
forming disks performed with iSHELL on the Infrared Telescope Facility, using two slits that …