activity
20132020
most citedA near-IR spectroscopic survey of massive jets towards EGOs

81 citations · 160 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2020★ 4 cited

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.SR2017★ 8 cited

Deep into the Water Fountains: The case of IRAS 18043-2116

A. F. Pérez-Sánchez, D. Tafoya, R. García López +2

(Abridged) The formation of large-scale (hundreds to few thousands of AU) bipolar structures in the circumstellar envelopes (CSEs) of post-Asymptotic Giant Branch (post-AGB) stars…

astro-ph.SR2016★ 2 cited

The innermost astronomical unit of protoplanetary disks

J. Kluska, R. Garcia Lopez, M. Benisty

Circumstellar disks around young stars are the birthsites of planets. It is thus fundamental to study the disks in which they form, their structure and the physical conditions ther…

astro-ph.SR2014★ 81 cited

A near-IR spectroscopic survey of massive jets towards EGOs

A. Caratti o Garatti, B. Stecklum, H. Linz +2

We aim at deriving the main physical properties of massive jets from near-IR observations, comparing them to those of a large sample of jets from low-mass YSOs, and relating them t…

astro-ph.SR2014★ 48 cited

POISSON project - III - Investigating the evolution of the mass accretion rate

S. Antoniucci, R. Garcia Lopez, B. Nisini +3

As part of the POISSON project (Protostellar Optical-Infrared Spectral Survey on NTT), we present the results of the analysis of low-resolution NIR spectra 0.9-2.4 um) of two sampl…

astro-ph.SR2013★ 17 cited

HD 85567: A Herbig B[e] star or an interacting B[e] binary

H. E. Wheelwright, G. Weigelt, A. Caratti o Garatti +1

Context. HD 85567 is an enigmatic object exhibiting the B[e] phenomenon, i.e. an infrared excess and forbidden emission lines in the optical. The object's evolutionary status is un…