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 41 publications
Deuterium Chemodynamics of Massive Pre-Stellar Cores
Hunting for Runaways from the Orion Nebula Cluster
Salt, Hot Water, and Silicon Compounds Tracing Massive Twin Disks
Stellar Variability in a Forming Massive Star Cluster
Gas Kinematics of the Massive Protocluster G286.21+0.17 Revealed by ALMA
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
The High-mass Protostellar Population of a Massive Infrared Dark Cloud
SiO emission as a probe of cloud-cloud collisions in infrared dark clouds
Dynamics of a massive binary at birth
An Ordered Envelope-Disk Transition in the Massive Protostellar Source G339.88-1.26
The SOFIA Massive (SOMA) Star Formation Survey. II. High Luminosity Protostars
Star cluster formation from turbulent clumps. II. Gradual star cluster formation
Multiple Feedback in Low-Metallicity Massive Star Formation
Disk Wind Feedback from High-mass Protostars
Interstellar Plunging Waves: ALMA Resolves the Physical Structure of Nonstationary MHD Shocks
Discovery of a Photoionized Bipolar Outflow toward the Massive Protostar G45.47+0.05
Measuring the ionisation fraction in a jet from a massive protostar
The Core Mass Function across Galactic Environments. II. Infrared Dark Cloud Clumps
The Core Mass Function in the Massive Protocluster G286.21+0.17 Revealed by ALMA
Fragmentation properties of massive protocluster gas clumps: an ALMA study
On the formation of runaway stars BN and x in the Orion Nebula Cluster
IN-SYNC. VIII. Primordial Disk Frequencies in NGC 1333, IC 348, and the Orion A Molecular Cloud
Zooming in to Massive Star Birth
High Spectral Resolution Observations toward Orion BN at 6 μm: No Evidence for Hot Water
Fire from Ice - Massive Star Birth from Infrared Dark Clouds
GMC Collisions as Triggers of Star Formation. IV. the Role of Ambipolar Diffusion
GMC Collisions as Triggers of Star Formation. V. Observational Signatures
Star Cluster Formation from Turbulent Clumps. I. The Fast Formation Limit
The Stellar Content of the Infalling Molecular Clump G286.21+0.17
Outflow-confined H II Regions. II. The Early Break-out Phase
Temperature structure and kinematics of the IRDC G035.39-00.33
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