Physical and Chemical Structure of the Disk and Envelope of the Class 0/I Protostar L1527
Author:
Funder
MORE RISE-to-PhD program
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/abd1db/pdf
Reference98 articles.
1. ANALYTICAL FORMULAE OF MOLECULAR ION ABUNDANCES AND THE N2H+RING IN PROTOPLANETARY DISKS
2. ALMA Observations of the Protostar L1527 IRS: Probing Details of the Disk and the Envelope Structures
3. Candidate solar-type protostars in nearby molecular cloud cores
4. The Effects of UV Continuum and Ly Radiation on the Chemical Equilibrium of T Tauri Disks
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1. Synthetic Observations of the Infalling Rotating Envelope: Links between the Physical Structure and Observational Features;The Astrophysical Journal;2024-01-01
2. Early Planet Formation in Embedded Disks (eDisk). III. A First High-resolution View of Submillimeter Continuum and Molecular Line Emission toward the Class 0 Protostar L1527 IRS;The Astrophysical Journal;2023-06-28
3. Filling in the gaps: can gravitationally unstable discs form the seeds of gas giant planets?;Monthly Notices of the Royal Astronomical Society;2023-05-24
4. Formation of Dust Clumps with Sub-Jupiter Mass and Cold Shadowed Region in Gravitationally Unstable Disk around Class 0/I Protostar in L1527 IRS;The Astrophysical Journal;2022-08-01
5. A likely flyby of binary protostar Z CMa caught in action;Nature Astronomy;2022-01-13
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