activity
20072021
most citedThe APOGEE-2 Survey of the Orion Star Forming Complex II: Six-dimensional structure

324 citations · 1.5k across the 33 of their papers we have counts for

collaborators

33 papers

astro-ph.SR2021★ 8 cited

Understanding the angular momentum evolution of T Tauri and Herbig Ae/Be stars

Giovanni Pinzón, Jesús Hernández, Javier Serna +8

We investigate a sample of 6 Herbig Ae/Be stars belonging to the Orion OB1 association, as well as 73 low mass objects, members of the Orionis cluster, in order to explore the…

astro-ph.GA2021★ 5 cited

The G 305 Star-forming Region: II. Irregular variable stars

N. Medina, J. Borissova, R. Kurtev +11

We present a catalog of 167 newly discovered, irregular variables spanning a 7 deg area that encompasses the G 305 star-forming complex, one of the most luminous giant…

astro-ph.GA2021★ 1 cited

Clustered star formation towards Berkeley 87 / ON2. I. Multi-wavelength census and the population overlap problem

Diego de la Fuente, Carlos G. Román-Zúñiga, Elena Jiménez-Bailón +3

(ABRIDGED) Disentangling line-of-sight alignments of young stellar populations is crucial for observational studies of star-forming complexes. This task is particularly problematic…

astro-ph.GA2019★ 14 cited

Not so different after all: Properties and Spatial Structure of Column Density Peaks in the Pipe and Orion A Clouds

Carlos G. Román-Zúñiga, Emilio Alfaro, Aina Palau +4

We present a comparative study of the physical properties and the spatial distribution of column density peaks in two Giant Molecular Clouds (GMC), the Pipe Nebula and Orion A, whi…

astro-ph.SR2019★ 29 cited

Flipping-up the field: gravitational feedback as a mechanism for young clusters dispersal

Manuel Zamora-Avilés, Javier Ballesteros-Paredes, Jesús Hernández +3

Recent analyses of Gaia data have provided direct evidence that most young stellar clusters are in a state of expansion, with velocities of the order of ~0.5 km/s. Traditionally, e…

astro-ph.SR2019★ 122 cited

Close companions around young stars

Marina Kounkel, Kevin Covey, Maxwell Moe +26

Multiplicity is a fundamental property that is set early during stellar lifetimes, and it is a stringent probe of the physics of star formation. The distribution of close companion…