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20082021
most citedA spectroscopic census in young stellar regions: the Sigma Orionis cluster

45 citations · 322 across the 19 of their papers we have counts for

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12 papers · 1 filter

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.SR2020★ 33 cited

The Evolution Of The Inner Regions of Protoplanetary Disks

Ezequiel Manzo-Martínez, Nuria Calvet, Jesús Hernández +6

We present a study of the evolution of the inner few astronomical units of protoplanetary disks around low-mass stars. We consider nearby stellar groups with ages spanning from 1 t…

astro-ph.SR2020★ 41 cited

Variable Accretion onto Protoplanet Host Star PDS 70

Thanawuth Thanathibodee, Brandon Molina, Nuria Calvet +6

The PDS 70 system has been subject to many studies in the past year following the discovery of two accreting planets in the gap of its circumstellar disk. Nevertheless, the mass ac…

astro-ph.SR2020★ 4 cited

Red Be stars in the Magellanic Clouds?

Katherine Vieira, Alejandro García-Varela, Beatriz Sabogal +2

We revisit the subject of Be star candidates towards the Magellanic Clouds, previously studied by the authors using SPM4 proper motions. We obtain GAIA DR2 parallaxes and proper mo…

astro-ph.SR2019★ 8 cited

A kinematically unbiased, all-sky search for nearby, young, low-mass stars

Alexander S. Binks, Matthieu Chalifour, Joel H. Kastner +6

The past two decades have seen dramatic progress in our knowledge of the population of young stars of age Myr that lie within pc of the Sun. These nearby, young sta…

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…