- Atacama Large Millimeter Submillimeter ArrayCL4 papers
- Center for Astrophysics Harvard & SmithsonianUS4 papers
- Institute of Astronomy and Astrophysics, Academia SinicaTW4 papers
- National Radio Astronomy ObservatoryUS4 papers
- Institut d'Estudis Espacials de CatalunyaES3 papers
- Institute of Space SciencesES3 papers
- Instituto Argentino de RadioastronomíaAR3 papers
- Korea Astronomy and Space Science InstituteKR3 papers
- Max Planck Institute for AstronomyDE3 papers
- National Astronomical Observatory of JapanJP3 papers
- Arcetri Astrophysical ObservatoryIT2 papers
- Institut de Radioastronomie MillimétriqueFR2 papers
4 papers · 1 filter
Magneto-Gravitational Regulated Streamer Accretion onto a Class 0 Protostellar System
Bo Huang, Josep M. Girart, Ian W. Stephens +17
How do magnetic fields shape the way young stars gather gas from their birth clouds? Using high-resolution Atacama Large Millimeter/submillimeter Array observations of a young trip…
The dominance of turbulence over magnetism in the formation of massive star cluster seeds
Junhao Liu, Patricio Sanhueza, Piyali Saha +32
High-mass stars form in protoclusters, where gravo-magnetic processes shape collapsing clouds and clumps to be elongated preferentially perpendicular to magnetic (B) fields. Yet it…
Magnetic field alignment with dense cores in the transition between cloud and core scales
Sean Yin, Ayush Pandhi, Rachel Friesen +7
In a magnetically-dominated model of star formation, we expect to see alignments between the magnetic field orientation of star-forming dense cores and the cloud-scale magnetic fie…
PRODIGE - envelope to disk with NOEMA: VII. (Complex) organic molecules in the NGC1333 IRAS4B1 outflow: A new laboratory for shock chemistry
Laura A. Busch, J. E. Pineda, P. Caselli +20
Shock chemistry is an excellent tool to shed light on the formation and destruction mechanisms of complex organic molecules (COMs). The L1157-mm outflow is the only low-mass protos…