PROtostars & DIsks: Global Evolution (PRODIGE) Archives

Cartoon highlighting the main molecular features of the IRAS4B1 outflow. The main emission morphology of our reference molecule, CH3OH, is outlined in grey, including the main outflow lobes (red and blue arrows) and additional arc-like features (black lines) of currently unknown origin. The peaks of the intensity ratios with respect to CH3OH are highlighted in teal and pink, depending on the species (see Fig. 2). A spectral line analysis was performed towards positions R1 and B1 and yielded rotational temperatures of Trot = 60-100 K (Sect. 3.3). The position of the protostar is indicated in yellow. -- Astronomy & Astrophysics

Astrochemistry, Astronomy & Telescopes, Biosignatures & Paleobiology, Imaging & Spectroscopy, Interstellar, Status Report

PRODIGE – Envelope To Disk With NOEMA VII. (Complex) Organic Molecules In The NGC1333 IRAS 4B1 Outflow: A New Laboratory For Shock Chemistry

by Keith CowingJune 9, 2026June 10, 2026

Context. Shock chemistry is an excellent tool for shedding light on the formation and destruction mechanisms of complex organic molecules (COMs). The L1157-mm outflow is the only low-mass protostellar outflow […]

PROtostars & DIsks: Global Evolution (PRODIGE)

PRODIGE – Envelope To Disk With NOEMA VII. (Complex) Organic Molecules In The NGC1333 IRAS 4B1 Outflow: A New Laboratory For Shock Chemistry

A Search For Narrowband Technosignatures From LTT 3780 With The Allen Telescope Array And The Karl G. Jansky Very Large Array

Tricorder Tech: Identifying Proteins, Molecule By Molecule

First Completed Rocky Worlds Program Observations Open New Era in Exoplanet Studies

Pioneer 10/11 Telemetry Explanatory Almanac

Diverse Organic Molecules Discovered Surrounding A Newly Formed Star