Jonathan Tan
Jonathan Tan is employed as Professor in the unit Galactic Astronomy, at the Division of Astronomy and Plasma Physics.
Tan is a theoretical astrophysicist, with a broad range of research interests in galaxy, star and planet formation. He is leading the new Chalmers Initiative on Cosmic Origins (CICO), see link below.
Jonathan Tan received his Ph.D. from UC Berkeley in 2001. He was a Lyman-Spitzer Postdoctoral Fellow and Lecturer at Princeton Univ. from 2001-2004, a Zwicky Postdoctoral Fellow at ETH Zurich from 2004-2005 and an Asst./Assoc. Prof. at Univ. of Florida from 2005-2017.
Showing 112 publications
Flash Ionization of the Early Universe by Population III.1 Supermassive Stars
The Core Mass Function across Galactic Environments. IV. The Galactic Center
Exploring Magnetic Fields in Molecular Clouds through Denoising Diffusion Probabilistic Models
The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows
ABYSS. III. Observing Accretion Activity in Young Stars Through Empirical Veiling Measurements
Discovery of Radio Recombination Lines from Proplyds in the Orion Nebula Cluster
Rotating supermassive Pop III stars on the main sequence
The SOFIA Massive (SOMA) Star Formation Survey. V. Clustered Protostars
The emergence and ionizing feedback of Pop III.1 stars as progenitors for supermassive black holes
Carbon-chain chemistry in the interstellar medium
Expansion kinematics of young clusters: I. Lambda Ori
Astrochemical Diagnostics of the Isolated Massive Protostar G28.20-0.05
Star cluster formation from turbulent clumps - IV. Protoplanetary disc evolution
Disk Wind Feedback from High-mass Protostars. III. Synthetic CO Line Emission
Disk Wind Feedback from High-mass Protostars. IV. Shock-ionized Jets
The Impact of Shear on Disk Galaxy Star Formation Rates
An HST Study of the Substellar Population of NGC 2024
GMC collisions as triggers of star formation – VIII. The core mass function
The SOFIA Massive (SOMA) Star Formation Survey. IV. Isolated Protostars
Star cluster formation from turbulent clumps – III. Across the mass spectrum
On the Lifetime of Molecular Clouds with the “Tuning-fork” Analysis
Spitzer thermal phase curve of WASP-121 b
Denoising Diffusion Probabilistic Models to Predict the Density of Molecular Clouds
Mother of dragons: A massive, quiescent core in the dragon cloud (IRDC G028.37+00.07)
Disk Wind Feedback from High-mass Protostars. II. The Evolutionary Sequence
Massive Protostars in a Protocluster—A Multi-scale ALMA View of G35.20-0.74N
A Census of Outflow to Magnetic Field Orientations in Nearby Molecular Clouds
Isolated Massive Star Formation in G28.20-0.05
Astrochemical modelling of infrared dark clouds
Inside-out planet formation: VI. oligarchic coagulation of planetesimals from a pebble ring?
The Disk Population in a Distant Massive Protocluster
The Hi-GAL compact source catalogue - II. The 360° catalogue of clump physical properties
Deuterium Chemodynamics of Massive Pre-Stellar Cores
The Core Mass Function across Galactic Environments. III. Massive Protoclusters
Is There Any Linkage between Interstellar Aldehyde and Alcohol?
MRI-active inner regions of protoplanetary discs. I. A detailed model of disc structure
Star cluster formation in Orion A
ALMA-IRDC: dense gas mass distribution from cloud to core scales
Star Formation in a Strongly Magnetized Cloud
Photodissociation region diagnostics across galactic environments
SiO Outflows as Tracers of Massive Star Formation in Infrared Dark Clouds
Hunting for Runaways from the Orion Nebula Cluster
SiO emission as a probe of cloud-cloud collisions in infrared dark clouds
An X-Ray View of Two Infrared Dark Clouds G034.43+00.24 and G035.39-00.33
The SOFIA Massive (SOMA) Star Formation Survey. III. From Intermediate- to High-mass Protostars
Gas Kinematics of the Massive Protocluster G286.21+0.17 Revealed by ALMA
The High-mass Protostellar Population of a Massive Infrared Dark Cloud
Salt, Hot Water, and Silicon Compounds Tracing Massive Twin Disks
Stellar Variability in a Forming Massive Star Cluster
Disk Wind Feedback from High-mass Protostars
Dynamics of a massive binary at birth
Star cluster formation from turbulent clumps. II. Gradual star cluster formation
The SOFIA Massive (SOMA) Star Formation Survey. II. High Luminosity Protostars
Measuring the ionisation fraction in a jet from a massive protostar
Interstellar Plunging Waves: ALMA Resolves the Physical Structure of Nonstationary MHD Shocks
Multiple Feedback in Low-Metallicity Massive Star Formation
Discovery of a Photoionized Bipolar Outflow toward the Massive Protostar G45.47+0.05
An Ordered Envelope-Disk Transition in the Massive Protostellar Source G339.88-1.26
IN-SYNC. VIII. Primordial Disk Frequencies in NGC 1333, IC 348, and the Orion A Molecular Cloud
Fragmentation properties of massive protocluster gas clumps: an ALMA study
High Spectral Resolution Observations toward Orion BN at 6 μm: No Evidence for Hot Water
The Core Mass Function across Galactic Environments. II. Infrared Dark Cloud Clumps
Zooming in to Massive Star Birth
The inception of star cluster formation revealed by [C ii] emission around an Infrared Dark Cloud
On the formation of runaway stars BN and x in the Orion Nebula Cluster
The Core Mass Function in the Massive Protocluster G286.21+0.17 Revealed by ALMA
GMC Collisions as Triggers of Star Formation. V. Observational Signatures
Fire from Ice - Massive Star Birth from Infrared Dark Clouds
Outflow-confined H II Regions. II. The Early Break-out Phase
GMC Collisions as Triggers of Star Formation. IV. the Role of Ambipolar Diffusion
The Stellar Content of the Infalling Molecular Clump G286.21+0.17
Star Cluster Formation from Turbulent Clumps. I. The Fast Formation Limit
Temperature structure and kinematics of the IRDC G035.39-00.33
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