Below a selection of publications with the main Results:

WP1

Task 1.1.: Accretion rates for a sample of young stars

Improving Accretion Diagnostics for Young Stellar Objects with Mid-infrared Hydrogen lines from JWST/MIRI

Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission

Coordinated Space- and Ground-based Monitoring of Accretion Bursts in a Protoplanetary Disk: Establishing Mid-infrared Hydrogen Lines as Accretion Diagnostics for JWST/MIRI

Revisiting empirical relations to measure accretion luminosity

A new approach to use class III spectra to derive stellar and accretion properties

Task 1.2: Outflow rates from line emission with JWST

The Structure and Kinematics of Three Class 0 Protostellar Jets from JWST

The Shocking H2 Outflow from HH 46

The [D/H] abundance derived from protostellar outflows across the Galactic disk measured with JWST

JWST Observations of Young protoStars (JOYS): HH211: Textbook case of a protostellar jet and outflow

JWST Observations of Young protoStars (JOYS): Overview of gaseous molecular emission and absorption in low-mass protostars

Investigating Protostellar Accretion-driven Outflows across the Mass Spectrum: JWST NIRSpec Integral Field Unit 3–5 μm Spectral Mapping of Five Young Protostars

JWST Observations of HH46 IRS and Its Outflow. Overview and First Results

Task 1.3: Disc population synthesis models under wind driven accretion

Testing Accretion Mechanisms from Disk Population Synthesis

The survivorship bias of protoplanetary disc populations: Internal photoevaporation causes an apparent increase in the median total disc mass with time

The Time Evolution of {M}_{d}/\dot{M} in Protoplanetary Disks as a Way to Disentangle between Viscosity and MHD Winds

WP2

Task 2.1: Measuring the disc mass dynamically from CO rotation curves with ALMA

exoALMA. I. Science Goals, Project Design, and Data Products

exoALMA. III. Line-intensity Modeling and System Property Extraction from Protoplanetary Disks

exoALMA. VI. Rotating under Pressure: Rotation Curves, Azimuthal Velocity Substructures, and Gas Pressure Variations

exoALMA. X. Channel Maps Reveal Complex 12CO Abundance Distributions and a Variety of Kinematic Structures with Evidence for Embedded Planets

exoALMA. XII. Weighing and Sizing exoALMA Disks with Rotation Curve Modelling

exoALMA. XIII. Gas Masses from N2H+ and C18O: A Comparison of Measurement Techniques for Protoplanetary Gas Disk Masses

Task 2.2: Measuring the “GI-wiggle” from ALMA kinematics and the likelihood of disc fragmentation

Infall-driven gravitational instability in accretion discs

exoALMA. XV. Interpreting the Height of CO Emission Layer

Task 2.3: Determining the role of GIs in the formation of planetesimals and planetary cores

Gravitational instability in a planet-forming disk

Angular momentum transport via gravitational instability in the Elias 2-27 disc

WP3

Task 3.1: Derive disc morphologies in multiple systems from SPHERE and ALMA imaging

The Corona-Australis star-forming region: New insights on its formation history from detailed stellar and disk analysis

Task 3.2: What's the impact of Kozai-Lidov oscillations to promote or inhibit polar disc alignment?

Brightness variability in polar circumbinary disks

Probing initial distributions of orbital eccentricity and disc misalignment via polar discs

Task 3.3: What's the origin of accretion outbursts in the embedded phase?

The role of thermal instability in accretion outbursts in high-mass stars

The accretion burst of the massive young stellar object G323.46−0.08

The most variable VVV sources: eruptive protostars, dipping giants in the nuclear disc and others

Radio outburst from a massive (proto)star. III. Unveiling the bipolarity of the radio jet from S255IR NIRS 3

Radio outburst from a massive (proto)star. II. A portrait in space and time of the expanding radio jet from S255IR NIRS 3

Link to publications

The project funded or co-funded more than 90 publications.

Clicking the link below you will find the list of publications and links to the papers funded by the PATH project:

https://ui.adsabs.harvard.edu/user/libraries/jL8vDuHfQjG-XtykYCZ0FA