activity
20032023
most citedChandra Orion Ultradeep Project: Observations and Source Lists

391 citations · 1.9k across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2023★ 36 cited

Herbig Stars: A Quarter Century of Progress

Sean D. Brittain, Inga Kamp, Gwendolyn Meeus +2

Herbig Ae/Be stars are young contracting stars on the radiative track in the HR diagram on their way to the main sequence. These stars provide a valuable link between high and low…

astro-ph.SR2022★ 17 cited

Relation between metallicities and spectral energy distributions of Herbig Ae/Be stars. A potential link with planet formation

J. Guzman-Diaz, B. Montesinos, I. Mendigutia +5

(Abridged) The stellar metallicity, [M/H], may have important implications for planet formation. In particular, Kama et al. proposed that the deficit of refractory elements in the…

astro-ph.EP2022★ 26 cited

A scaled-up planetary system around a supernova progenitor

V. Squicciarini, R. Gratton, M. Janson +24

Virtually all known exoplanets reside around stars with ; to clarify if the dearth of planets around more massive stars is real, we launched the direct-imaging B-sta…

astro-ph.SR2021★ 5 cited

The A-shell star Phi Leo revisited: its photospheric and circumstellar spectra

C. Eiroa, B. Montesinos, I. Rebollido +7

Variable red- and blue-shifted absorption features observed in the Ca ii K line towards the A-type shell star Leo have been suggested by us in a previous work to be likely due…

astro-ph.SR2020★ 71 cited

The Evolution of Disk Winds from a Combined Study of Optical and Infrared Forbidden Lines

I. Pascucci, A. Banzatti, U. Gorti +18

We analyze high-resolution (dv=<10km/s) optical and infrared spectra covering the [OI] 6300 angstrom and [NeII] 12.81 micron lines from a sample of 31 disks in different evolutiona…

astro-ph.SR2018★ 38 cited

The co-existence of hot and cold gas in debris discs

I. Rebollido, C. Eiroa, B. Montesinos +19

Debris discs have often been described as gas-poor discs as the gas-to-dust ratio is expected to be considerably lower than in primordial,protoplanetary discs. However, recent obse…