77 citations · 294 across the 60 of their papers we have counts for
6 papers · 1 filter
HI content at cosmic noon -- a millimeter-wavelength perspective
Hugo Messias, Andrea Guerrero, Neil Nagar +4
In order to understand galaxy growth evolution, it is critical to constrain the evolution of its building block: gas. Mostly comprised by Hydrogen in its neutral (HI) and molecular…
Gaia uncovers difference in B and Be star binarity at small scales: evidence for mass transfer causing the Be phenomenon
Jonathan M. Dodd, René D. Oudmaijer, Isaac C. Radley +2
Be stars make up almost 20% of the B star population, and are rapidly rotating stars surrounded by a disc; however the origin of this rotation remains unclear. Mass transfer within…
Clustering properties of intermediate and high-mass Young Stellar Objects
Miguel Vioque, Manuel Cavieres, Michelangelo Pantaleoni González +6
We have selected 337 intermediate and high-mass YSOs ( to M) well-characterised with spectroscopy. By means of the clustering algorithm HDBSCAN, we study their…
The -- relationship for Herbig Ae/Be stars: a lifetime problem for disks with low masses?
Sierra L. Grant, Lucas M. Stapper, Michiel R. Hogerheijde +3
The accretion of material from protoplanetary disks onto their central stars is a fundamental process in the evolution of these systems and a key diagnostic in constraining the dis…
The Radial Distribution and Excitation of H2 around Young Stars in the HST-ULLYSES Survey
Kevin France, Nicole Arulanantham, Erin Maloney +8
The spatial distribution and evolution of gas in the inner 10 au of protoplanetary disks form the basis for estimating the initial conditions of planet formation. Among the most im…
Large Myr-old Disks are Not Severely Depleted of gas-phase CO or carbon
Ilaria Pascucci, Bennett N. Skinner, Dingshan Deng +6
We present an ACA search for [CI] emission at 492GHz toward large T Tauri disks (gas radii au) in the Myr-old Lupus star-forming region. Combined with ALMA 1…