309 citations
- Center for Astrophysics Harvard & SmithsonianUS11 papers
- University of Illinois Urbana-ChampaignUS7 papers
- University of VirginiaUS7 papers
- Pennsylvania State UniversityUS6 papers
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- Université Bourgogne Franche-ComtéFR6 papers
- University College LondonGB6 papers
- Carnegie Mellon UniversityUS5 papers
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- Max Planck Institute for AstronomyDE5 papers
- National Astronomical Observatory of JapanJP5 papers
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7 papers · 1 filter
Evolution and Kinematics of Protostellar Envelopes in the Perseus Molecular Cloud
Daniel J. Heimsoth, Ian W. Stephens, Hector G. Arce +3
We present a comprehensive analysis on the evolution of envelopes surrounding protostellar systems in the Perseus molecular cloud using data from the MASSES survey. We focus our at…
Thermal Emission and Scattering by Aligned Grains: Plane-Parallel Model and Application to Multiwavelength Polarization of the HL Tau Disk
Zhe-Yu Daniel Lin, Zhi-Yun Li, Haifeng Yang +4
Telescopes are now able to resolve dust polarization across circumstellar disks at multiple wavelengths, allowing the study of the polarization spectrum. Most disks show clear evid…
Mixed Reality using Illumination-aware Gradient Mixing in Surgical Telepresence: Enhanced Multi-layer Visualization
Nirakar Puri, Abeer Alsadoon, P. W. C. Prasad +2
Background and aim: Surgical telepresence using augmented perception has been applied, but mixed reality is still being researched and is only theoretical. The aim of this work is…
The Transition of Polarized Dust Thermal Emission from the Protostellar Envelope to the Disk Scale
Ka Ho Lam, Che-Yu Chen, Zhi-Yun Li +4
Polarized dust continuum emission has been observed with ALMA in an increasing number of deeply embedded protostellar systems. It generally shows a sharp transition going from the…
HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure
Dennis Lee, Marc Berthoud, Che-Yu Chen +14
We present a study of the relative orientation between the magnetic field and elongated cloud structures for the Oph A and Oph E regions in L1688 in the Ophiuchus molecular…
Gravity Driven Magnetic Field at ~1000 au Scales in High-mass Star Formation
Patricio Sanhueza, Josep Miquel Girart, Marco Padovani +20
A full understanding of high-mass star formation requires the study of one of the most elusive components of the energy balance in the interstellar medium: magnetic fields. We repo…