Jonas Syed

Max-Planck-Institut für Astronomie

Germany

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Articles (11)

Year:

2024

Year:

2023

Year:

2023

Year:

2022

Year:

2022

Year:

2022

Year:

2022

Year:

2021

Year:

2021

Year:

2020

Year:

2020

Collaborators (7)

Juan Diego Soler

Istituto Nazionale di Astrofisica

ITALY

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Jeroen Stil

Associate Professor

University of Calgary

CANADA

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Philipp Girichidis

Heidelberg University

GERMANY

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Henrik Beuther

Max-Planck-Institut für Astronomie

GERMANY

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Thomas Möller

University of Cologne

GERMANY

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Daniel Apai

Professor

University of Arizona

UNITED STATES

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Gary Fuller

The University of Manchester

UNITED KINGDOM

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Jonas Syed

Research Interests

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Articles (11)

Dynamical accretion flows

EDEN Survey: Small Transiting Planet Detection Limits and Constraints on the Occurrence Rates of Planets around Late-M Dwarfs within 15 pc

Cold atomic gas identified by H I self-absorption

Properties of atomic hydrogen gas in the Galactic plane from THOR 21-cm absorption spectra: a comparison with the high latitude gas

Polarized Emission from Four Supernova Remnants in the THOR Survey

On the accuracy of H i observations in molecular clouds – More cold H i than thought?

The “Maggie” filament: Physical properties of a giant atomic cloud

The filamentary structures in the CO emission toward the Milky Way disk

Fragmentation and kinematics in high-mass star formation

Atomic and molecular gas properties during cloud formation

The history of dynamics and stellar feedback revealed by the H I filamentary structure in the disk of the Milky Way

Collaborators (7)

Juan Diego Soler

Jeroen Stil

Philipp Girichidis

Henrik Beuther

Thomas Möller

Daniel Apai

Gary Fuller

Make your next move.

Jonas Syed

Research Interests

Explore related searches

Contact this professor

Articles (11)

Dynamical accretion flows

EDEN Survey: Small Transiting Planet Detection Limits and Constraints on the Occurrence Rates of Planets around Late-M Dwarfs within 15 pc

Cold atomic gas identified by H I self-absorption

Properties of atomic hydrogen gas in the Galactic plane from THOR 21-cm absorption spectra: a comparison with the high latitude gas

Polarized Emission from Four Supernova Remnants in the THOR Survey

On the accuracy of H i observations in molecular clouds – More cold H i than thought?

The “Maggie” filament: Physical properties of a giant atomic cloud

The filamentary structures in the CO emission toward the Milky Way disk

Fragmentation and kinematics in high-mass star formation

Atomic and molecular gas properties during cloud formation

The history of dynamics and stellar feedback revealed by the H I filamentary structure in the disk of the Milky Way

Collaborators (7)

Juan Diego Soler

Jeroen Stil

Philipp Girichidis

Henrik Beuther

Thomas Möller

Daniel Apai

Gary Fuller

Make your next move.

Cold atomic gas identified by H I self-absorption

The history of dynamics and stellar feedback revealed by the H I filamentary structure in the disk of the Milky Way