85 citations · 384 across the 11 of their papers we have counts for
12 papers
Chemistry on solar system scales
Catherine Walsh, Maria Drozdovskaya, Dmitry Semenov +33
The initial chemical composition of planets, primitive bodies in our solar system, and exoplanets is ultimately set by their nascent protoplanetary disks. Yet observing key carbon-…
SHARPing accretion and outflows in young stellar objects in star forming regions of the outer Galaxy and beyond
Juan Manuel Alcala', Alessio Caratti o Garatti, Linda Podio +5
As part of the science book of SHARP, we present here the science case of star-disk interaction of low-mass (\Mstar2\Msun) young stellar objects (YSOs), in low-metallicity (Z…
Organic chemistry in the protosolar analogue HOPS-108: Environment matters
L. Chahine, A. López-Sepulcre, R. Neri +10
Hot corinos are compact regions around solar-mass protostellar objects that are very rich in interstellar complex organic molecules (iCOMs). They are believed to represent the very…
The CALYPSO IRAM-PdBI survey of jets from Class 0 protostars. Are jets ubiquitous in young stars ?
L. Podio, B. Tabone, C. Codella +10
As a part of the CALYPSO large programme, we constrain the properties of protostellar jets and outflows in a sample of 21 Class 0 protostars with internal luminosities, Lint, from…
Silicon-bearing molecules in the shock L1157-B1: first detection of SiS around a Sun-like protostar
L. Podio, C. Codella, B. Lefloch +9
The shock L1157-B1 driven by the low-mass protostar L1157-mm is an unique environment to investigate the chemical enrichment due to molecules released from dust grains. IRAM-30m an…
Water and acetaldehyde in HH212: The first hot corino in Orion
C. Codella, C. Ceccarelli, S. Cabrit +7
Aims: Using the unprecedented combination of high resolution and sensitivity offered by ALMA, we aim to investigate whether and how hot corinos, circumstellar disks, and ejected ga…
Complex organic molecules in protostellar environments in the SKA era
C. Codella, L. Podio, F. Fontani +10
Molecular complexity builds up at each step of the Sun-like star formation process, starting from simple molecules and ending up in large polyatomic species. Complex organic molecu…
ESO-H~574 and Par-Lup3-4 Jets: Exploring the spectral, kinematical and physical properties
E. T. Whelan, R. Bonito, S. Antoniucci +7
In this paper a comprehensive analysis of VLT / X-Shooter observations of two jet systems, namely ESO-H 574 a K8 classical T Tauri star and Par-Lup 3-4 a very low mass (0.13~\Ms…
[OI] disk emission in the Taurus star forming region
G. Aresu, I. Kamp, R. Meijerink +8
The structure of protoplanetary disks is thought to be linked to the temperature and chemistry of their dust and gas. Whether the disk is flat or flaring depends on the amount of r…
Herschel/PACS observations of young sources in Taurus: the far-infrared counterpart of optical jets
L. Podio, I. Kamp, D. Flower +8
Observations of the atomic and molecular line emission associated with jets and outflows emitted by young stellar objects can be used to trace the various evolutionary stages they…
Gas in Protoplanetary Discs (GASPS) 1. First results
G. S. Mathews, W. R. F. Dent, J. P. Williams +50
Context - Circumstellar discs are ubiquitous around young stars, but rapidly dissipate their gas and dust on timescales of a few Myr. The Herschel space observatory allows for the…
Physical Structure and Dust Reprocessing in a sample of HH Jets
L. Podio, S. Medves, F. Bacciotti +2
We investigate the physical structure and dust reprocessing in the shocks along the beam of a number of classical Herbig-Haro jets in the Orion and Lupus molecular cloud. Spectral…