activity
20182022
most citedA measure of the size of the magnetospheric accretion region in TW Hydrae

42 citations · 99 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph.SR202142 cited

A measure of the size of the magnetospheric accretion region in TW Hydrae

R. Garcia Lopez, A. Natta, A. Caratti o Garatti +69

Stars form by accreting material from their surrounding disks. There is a consensus that matter flowing through the disk is channelled onto the stellar surface by the stellar magne…

astro-ph.SR20202 cited

The GRAVITY Young Stellar Object survey IV. The CO overtone emission in 51 Oph at sub-au scales

GRAVITY Collaboration, M. Koutoulaki, R. Garcia Lopez +69

51 Oph is a Herbig Ae/Be star that exhibits strong near-infrared CO ro-vibrational emission at 2.3 micron, most likely originating in the innermost regions of a circumstellar disc.…

astro-ph.SR2020

Investigating episodic accretion in a very low-mass young stellar object

Camille Stock, Alessio Caratti o Garatti, Pauline McGinnis +4

Very low-mass Class I protostars have been investigated very little thus far. Variability of these young stellar objects (YSOs) and whether or not they are capable of strong episod…

astro-ph.GA2020

The SOFIA Massive (SOMA) Star Formation Survey. III. From Intermediate- to High-Mass Protostars

Mengyao Liu, Jonathan C. Tan, James M. De Buizer +9

We present m SOFIA-FORCAST images of 14 intermediate-mass protostar candidates as part of the SOFIA Massive (SOMA) Star Formation Survey. We build spectral energy dis…

astro-ph.SR2020

The GRAVITY young stellar object survey. II. First spatially resolved observations of the CO bandhead emission in a high-mass YSO

GRAVITY Collaboration, A. Caratti o Garatti, R. Fedriani +50

The inner regions of the discs of high-mass young stellar objects (HMYSOs) are still poorly known due to the small angular scales and the high visual extinction involved. We deploy…

astro-ph.SR2020

Mirror, mirror on the outflow cavity wall. Near-infrared CO overtone disc emission of the high-mass YSO IRAS 11101-5829

R. Fedriani, A. Caratti o Garatti, M. Koutoulaki +7

Aims: The inner regions of high-mass protostars are often invisible in the near-infrared. We aim to investigate the inner gaseous disc of IRAS11101-5829 through scattered light fro…