activity
20112021
most citedCatalogue of new Herbig Ae/Be and classical Be stars. A machine learning approach to Gaia DR2

77 citations · 231 across the 7 of their papers we have counts for

collaborators

13 papers

astro-ph.SR202116 cited

HS observations in young stellar disks in Taurus

P. Rivière-Marichalar, A. Fuente, R. Le Gal +7

Context. Studying gas chemistry in protoplanetary disks is key to understanding the process of planet formation. Sulfur chemistry in particular is poorly understood in interstellar…

astro-ph.SR20219 cited

K-band GRAVITY/VLTI interferometry of "extreme" Herbig Be stars. The size-luminosity relation revisited

P. Marcos-Arenal, I. Mendigutía, E. Koumpia +7

(Abridged:) It has been hypothesized that the location of Herbig Ae/Be stars (HAeBes) within the empirical relation between the inner disk radius (r), inferred from K-band i…

astro-ph.SR2021

PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis

C. F. Manara, A. Frasca, L. Venuti +69

The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…

astro-ph.SR20206 cited

Discovery of a jet from the single HAe/Be star HD 100546

P. C. Schneider, C. Dougados, E. T. Whelan +6

Young accreting stars drive outflows that collimate into jets, which can be seen hundreds of au from their driving sources. Accretion and outflow activity cease with system age, an…

astro-ph.SR202029 cited

On the Mass Accretion Rates of Herbig Ae/Be Stars. Magnetospheric Accretion or Boundary Layer?

I. Mendigutía

Understanding how young stars gain their masses through disk-to-star accretion is of paramount importance in astrophysics. It affects our knowledge about the early stellar evolutio…

astro-ph.SR202077 cited

Catalogue of new Herbig Ae/Be and classical Be stars. A machine learning approach to Gaia DR2

M. Vioque, R. D. Oudmaijer, M. Schreiner +4

The intermediate-mass pre-main sequence Herbig Ae/Be stars are key to understanding the differences in formation mechanisms between low- and high-mass stars. The study of the gener…