Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR2.7k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR2.4k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR2.3k papers
- Charles UniversityCZ2.3k papers
- Institute for High Energy PhysicsES2.3k papers
- Institut de Recherche sur les Lois Fondamentales de l'UniversFR2.2k papers
- The Ohio State UniversityUS2.1k papers
- Universidad Autónoma de MadridES2.1k papers
- Rutherford Appleton LaboratoryGB2.1k papers
- European Organization for Nuclear ResearchCH2.1k papers
- University of Wisconsin–MadisonUS2.1k papers
- Joint Institute for Nuclear ResearchRU2k papers
8 papers · 2 filters
Magnetic Field Strengths in Photodissociation Regions
Dana S. Balser, D. Anish Roshi, S. Jeyakumar +3
We measure carbon radio recombination line (RRL) emission at 5.3 GHz toward four HII regions with the Green Bank Telescope (GBT) to determine the magnetic field strength in the pho…
Finding Distant Galactic HII Regions
L. D. Anderson, W. P. Armentrout, B. M. Johnstone +4
The WISE Catalog of Galactic HII Regions contains HII region candidates lacking ionized gas spectroscopic observations. All candidates have the characteristic HII region…
Untangling the Recombination Line Emission from HII Regions with Multiple Velocity Components
L. D. Anderson, L. A. Hough, T. V. Wenger +2
HII regions are the ionized spheres surrounding high-mass stars. They are ideal targets for tracing Galactic structure because they are predominantly found in spiral arms and have…
Bipolar HII regions - Morphology and star formation in their vicinity - I - G319.8800.79 and G010.3200.15
L. Deharveng, A. Zavagno, M. R. Samal +9
Our goal is to identify bipolar HII regions and to understand their morphology, their evolution, and the role they play in the formation of new generations of stars. We use the Spi…
Azimuthal Metallicity Structure in the Milky Way Disk
Dana S. Balser, Trey V. Wenger, L. D. Anderson +1
Elemental abundance patterns in the Galactic disk constrain theories of the formation and evolution of the Milky Way. HII region abundances are the result of billions of years of c…
Tracing the Conversion of Gas into Stars in Young Massive Cluster Progenitors
D. L. Walker, S. N. Longmore, N. Bastian +5
Whilst young massive clusters (YMCs; 10 M, age 100 Myr) have been identified in significant numbers, their progenitor gas clouds have elude…
A cluster in the making: ALMA reveals the initial conditions for high-mass cluster formation
J. M. Rathborne, S. N. Longmore, J. M. Jackson +9
G0.253+0.016 is a molecular clump that appears to be on the verge of forming a high mass, Arches-like cluster. Here we present new ALMA observations of its small-scale (~0.07 pc) 3…
Interferometric Observations of High-Mass Star-Forming Clumps with Unusual N2H+/HCO+ Line Ratios
Ian W. Stephens, James M. Jackson, Patricio Sanhueza +4
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey has detected high-mass star-forming clumps with anomalous NH/HCO(1-0) integrated intensity ratios that are e…