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Interstellar Medium

Interstellar medium both in the Milky Way and other galaxies

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Star Formation

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Disks

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Asteroids

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Asteroids

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Asteroids

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Asteroids

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About Us

ISM Group Members at Kapteyn Astronomical Institute and
SRON - Netherlands Institute for Space Research

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Prof. Dr. Floris F. S. van der Tak

Personal Webpage
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Prof. Dr. Inga Kamp

Personal Webpage
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Dr. Russell Shipman

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Dr. Fred Lahuis

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Dr. Michael "Migo" Mueller

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Dr. Christian Rab

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Aaron Greenwood MSc

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Kateryna Frantseva MSc

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William J. Pearson MSci

Personal Webpage
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Umit Kavak MSc

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Nick Oberg MSc

Projects

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Prof. Dr. Floris F.S. van der Tak

Email / Personal Website

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Prof. Dr. Inga Kamp

Email / Personal Website

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Dr. Russell Shipman

Email / Personal Website

Latest Publications

The papers which have been published by ISM Group Members

Deep Learning for Galaxy Mergers in the Galaxy Main Sequence

22
Jan, 2019

Starburst galaxies are often found to be the result of galaxy mergers. As a result, galaxy mergers are often believed to lie above the galaxy main sequence: the tight correlation between stellar mass and star formation rate. Here, we aim to test this claim. Deep learning techniques are applied ...

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Episodic excursions of low-mass protostars on the Hertzsprung-Russell diagram

28
Dec, 2018

Following our recent work devoted to the effect of accretion on the pre-main-sequence evolution of low-mass stars, we perform a detailed analysis of episodic excursions of low-mass protostars in the Hertzsprung-Russell (H-R) diagram triggered by strong mass accretion bursts typical of FU Orioni...

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Warm dust surface chemistry. H2 and HD formation

17
Dec, 2018

Molecular hydrogen (H2) is the main constituent of the gas in the planet-forming disks that surround many PMS stars. H2 can be incorporated in the atmosphere of the giant planets. HD has been detected in a few disks and can be considered the most reliable tracer of H2. We wish to form H2 and HD...

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Contact

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