activity
20142022
most citedGas and dust in the Beta Pictoris Moving Group as seen by the Herschel Space Observatory

86 citations · 337 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR202242 cited

Towards a comprehensive view of accretion, inner disks, and extinction in classical T Tauri stars: an ODYSSEUS study of the Orion OB1b association

Caeley V. Pittman, Catherine C. Espaillat, Connor E. Robinson +21

The coevolution of T Tauri stars and their surrounding protoplanetary disks dictates the timescales of planet formation. In this paper, we present magnetospheric accretion and inne…

astro-ph.SR201664 cited

A spectroscopic survey of Herbig Ae/Be stars with X-Shooter II: Accretion diagnostic lines

John R Fairlamb, Rene D Oudmaijer, Ignacio Mendigutia +2

The Herbig Ae/Be stars (HAeBes) allow an exploration of the properties of Pre-Main Sequence(PMS) stars above the low-mass range () and those bordering…

astro-ph.SR201632 cited

The compact H emitting regions of the Herbig Ae/Be stars HD 179218 and HD 141569 from CHARA spectro-interferometry

I. Mendigutía, R. D. Oudmaijer, D. Mourard +1

This work presents CHARA/VEGA H spectro-interferometry (R ~ 6000, and /2B ~ 1 mas) of HD 179218 and HD 141569, doubling the sample of Herbig Ae/Be (HAeBe) stars for which thi…

astro-ph.SR201473 cited

Investigating the inner discs of Herbig Ae/Be stars with CO bandhead and Br Gamma emission

John D. Ilee, John Fairlamb, Rene D. Oudmaijer +4

Herbig Ae/Be stars lie in the mass range between low and high mass young stars, and therefore offer a unique opportunity to observe any changes in the formation processes that may…

astro-ph.SR201440 cited

Stellar parameters and accretion rate of the transition disk star HD 142527 from X-Shooter

I. Mendigutía, J. Fairlamb, B. Montesinos +4

HD 142527 is a young pre-main sequence star with properties indicative of the presence of a giant planet or/and a low-mass stellar companion. We have analyzed an X-Shooter/Very Lar…

astro-ph.SR201486 cited

Gas and dust in the Beta Pictoris Moving Group as seen by the Herschel Space Observatory

P. Riviere-Marichalar, D. Barrado, B. Montesinos +11

Context. Debris discs are thought to be formed through the collisional grinding of planetesimals, and can be considered as the outcome of planet formation. Understanding the proper…