29 citations · 68 across the 6 of their papers we have counts for
6 papers
SOFIA and ALMA Investigate Magnetic Fields and Gas Structures in Massive Star Formation: The Case of the Masquerading Monster in BYF 73
Peter J. Barnes, Stuart D. Ryder, Giles Novak +4
We present SOFIA+ALMA continuum and spectral-line polarisation data on the massive molecular cloud BYF 73, revealing important details about the magnetic field morphology, gas stru…
Linking High- and Low-Mass Star Formation: Observation-Based Continuum Modelling and Physical Conditions
R. L. Pitts, L. E. Kristensen, J. K. Jørgensen +1
Astronomers have yet to establish whether high-mass protostars form from high-mass prestellar cores, similar to their lower-mass counterparts, or from lower-mass fragments at the h…
Census of High- and Medium-mass Protostars V. CO Abundance and the Galactic Factor
Rebecca L. Pitts, Peter J. Barnes
We present the second dust continuum data release in the Census of High- and Medium-mass Protostars (CHaMP), expanding the methodology trialed in Pitts et al. 2019 to the entire CH…
Gemini, SOFIA, and ATCA Reveal Very Young, Massive Protostars in the Collapsing Molecular Cloud BYF 73
Rebecca L. Pitts, Peter J. Barnes, Stuart D. Ryder +1
We present multi-wavelength data on the globally infalling molecular cloud/protostellar cluster BYF 73. These include new far-IR spectral line and continuum data from SOFIA's Far I…
On the Diagnostic Power of FIR/Sub-mm SED Fitting in Massive Galactic Molecular Clumps
Rebecca L. Pitts, Peter J. Barnes, Frank Varosi
We used FIR and submillimeter continuum data from Herschel and the Atacama Pathfinder EXperiment (APEX) to fit pixel-by-pixel modified Planck SEDs to prestellar and protostellar cl…
The Galactic Census of High- and Medium-mass Protostars. IV. Molecular Clump Radiative Transfer, Mass Distributions, Kinematics, and Dynamical Evolution
Peter J. Barnes, Audra K. Hernandez, Erik Muller +1
We present CO, CO, and CO data as the next major release for the CHaMP project, an unbiased sample of Galactic molecular clouds in = 280-300$^{\c…