8k citations
- California Institute of TechnologyUS1.2k papers
- Center for Astrophysics Harvard & SmithsonianUS1.1k papers
- Centre National de la Recherche ScientifiqueFR951 papers
- Max Planck Institute for Radio AstronomyDE915 papers
- University of VirginiaUS756 papers
- Max Planck Institute for AstronomyDE712 papers
- European Southern ObservatoryCL684 papers
- Leiden UniversityNL568 papers
- Goddard Space Flight CenterUS505 papers
- Commonwealth Scientific and Industrial Research OrganisationAU502 papers
- University of California, BerkeleyUS499 papers
- University of ArizonaUS477 papers
5,671 papers
Magnetic Fields in Massive Star-forming Regions (MagMaR). IX. Radiative Torque Alignment and Disruption in NGC6334I
Vineet Rawat, Thiem Hoang, Patricio Sanhueza +18
Intense radiation from high-mass stars is expected to significantly affect dust grain alignment and evolution through RAdiative Torques (RATs). We investigate this effect in a mass…
The Neutral Atomic Hydrogen in the solar neighborhood (NeAtHood) project I. Ghost in the shell: Neutral atomic hydrogen in the extended Orion nebula
J. D. Soler, H. Beuther, S. C. O. Glover +15
The Orion Nebula is the nearest site of ongoing and recent high-mass star formation. It is a unique laboratory for studying the mass, energy, and momentum input from high-mass star…
ACES VII. Compact Continuum Source Catalog of the Central Molecular Zone
Jennifer Wallace, Cara Battersby, Nazar Budaiev +58
The Central Molecular Zone (CMZ) resides in the inner few hundred parsecs of our Galaxy, and despite being the largest reservoir of dense molecular gas in the Milky Way, it has a r…
The ALMA EGO-10 Survey of Massive Protoclusters: Correlation of 1.3 mm Continuum Source Clustering with Evolutionary State
Michael C. Logue, Claudia J. Cyganowski, Crystal L. Brogan +4
Massive stars characteristically form in clustered environments. Characterising young massive 'protoclusters' is therefore crucial to constraining the mechanism(s) of massive star…
Nascent Embedded-protostar Survey in Taurus (NEST) I: Protostellar Multiplicity
Aislinn C. Plante, John J. Tobin, Patrick D. Sheehan +5
We present new ALMA 0.9 mm and VLA 9 mm observations in the Taurus Molecular Cloud (TMC) of 25 protostellar systems, containing 40 protostars, observed at 0.3" (~20 au) resolution.…
Investigating anomalous microwave emission near G107.2+5.20 in Ku-band with the Green Bank Telescope
Jordan E. Shroyer, Bradley R. Johnson, Dillon J. Bass +5
Anomalous microwave emission (AME) is 30 GHz-peaking continuum emission thought to arise from spinning dust grains. Observations suggest that the local environment shapes the AME s…