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Zhe-Yu Daniel

As seen in: arXiv, Oxford University Press (OUP)
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Articles by Zhe-Yu Daniel

Astrophysics > Instrumentation and Methods for Astrophysics

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By Zhe-Yu Daniel, Josep Miquel
| arXiv
Polarization reveals details of circumstellar disks that are not readily available from total intensity observations. Via multi-wavelength polarimetric observations of disks, we can trace how planets form, how dust grains evolve at the onset of planet formation, and how magnetic fields (B-fields) influence accretion.
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Astrophysics > Earth and Planetary Astrophysics

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By Sidhant Kumar, Zhe-Yu Daniel
| arXiv
arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs.
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Astrophysics > Earth and Planetary Astrophysics

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By Zhe-Yu Daniel, Romane Le, L. Ilsedore
| arXiv
[Submitted on 8 Sep 2026 ( v1 ), last revised 5 Oct 2026 (this version, v2)] Title:The ALMA View of the Edge-on Gomez's Hamburger System: A Highly-Dynamic, Asymmetric Protoplanetary Disk Reveals the Earliest Phases of Giant Planet Formation Authors:Charles J. Law , Jensen Lawrence , Richard Teague , Zhe-Yu Daniel Lin , Romane Le Gal , Kristina Monsch , Gordian Edenhofer , Hans Baehr , Edwin A. Bergin , L. Ilsedore Cleeves , Anne Dutrey , Coralie Foucher , St├ęphane Guilloteau , Thomas J.
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Early Planet Formation in Embedded Disks (eDisk) XVI: An asymmetric dust disk driving a multi-component molecular outflow in the young Class 0 protostar GSS30 IRS3

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By de Gregorio-Monsalvo, Zhe-Yu Daniel, Chang Won
| arXiv
[Submitted on 30 Jul 2024] Title:Early Planet Formation in Embedded Disks (eDisk) XVI: An asymmetric dust disk driving a multi-component molecular outflow in the young Class 0 protostar GSS30 IRS3 Authors:Alejandro Santamaria-Miranda , Itziar de Gregorio-Monsalvo , Nagayoshi Ohashi , John J. Tobin , Jinshi Sai , Jes K. Jorgensen , Yusuke Aso , Zhe-Yu Daniel Lin , Christian Flores , Miyu Kido , Patrick M. Koch , Woojin Kwon , Chang Won Lee , Zhi-Yun Li , Leslie W. Looney , Adele L.
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Panchromatic (Sub)millimeter Polarization Observations of HL Tau Unveil Aligned Scattering Grains

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By CCT-La Plata, Villa Elisa, PO Box O, Zhe-Yu Daniel
| Oxford University Press (OUP)
Polarization is a unique tool to study the dust grains of protoplanetary disks. Polarization around HL Tau was previously imaged using the Atacama Large Millimeter/submillimeter Array (ALMA) at Bands 3 (3.1 mm), 6 (1.3 mm), and 7 (0.87 mm), showing that the polarization orientation changes across wavelength λ. Polarization at Band 7 is predominantly parallel to the disk minor axis but appears azimuthally oriented at Band 3, with the morphology at Band 6 in between the two.
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