Interstellar Medium
Interstellar medium both in the Milky Way and other galaxies
Star Formation
Low and Massive Star Formation in the Galaxy and star formation activity
Disks in Star Forming Regions
Disk formation and their chemical and physical evolution in star forming regions
Asteroids
The formation of asteroids and their role in space and life
Planet and Satellite Formation
The formation of planets and their moons using numerical models and observations
Receivers
Bolometers and Heterodyne receivers with the collaboration of SRON
Exoplanets and Astrobiology
The atmosphere of exoplanets and life in space
About Us
ISM Group Members at Kapteyn Astronomical Institute and
SRON - Netherlands Institute for Space Research
Dr. Russell Shipman
Dr. Fred Lahuis
Dr. Michael "Migo" Mueller
Dr. Christian Rab
Kateryna Frantseva MSc
Projects
DIANA Project
DIANA is an European Framework Seven (FP7) project, SPACE-2011 collaboration, project no 284405, which conducts a systematic collection and coherent analysis of observational data from the birth-places of extrasolar planets, the so-called protoplanetary discs. DIANA stands for DIscANAlysis.
SAFARI/SPICA Project
SPICA is a joint European-Japanese project under phase-A study at ESA: an infrared space observatory with a large, cryogenically cooled telescope. One of the instruments on board is SAFARI, a far-IR spectrometer providing instantaneously wavelength coverage of the 34 to 230 micron domain. One of the core objectives of this mission is to trace the gas, dust and ice evolution in planetary systems.
Latest Publications
The papers which have been published by ISM Group Members
Enrichment of the HR 8799 planets by minor bodies and dust
May, 2020
In the Solar System, minor bodies and dust deliver various materials to planetary surfaces. Several exoplanetary systems are known to host inner and outer belts, analogues of the main asteroid belt and the Kuiper belt. We study the possibility that exominor bodies and exodust deliver volatiles ...
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Gas and dust cooling along the major axis of M33 (HerM33es) -- Herschel/PACS [CII] and [OI] observations
May, 2020
M33 is a gas rich spiral galaxy of the Local Group. We investigate the relationship between the two major gas cooling lines and the total infrared (TIR) dust continuum. We mapped the emission of gas and dust in M33 using the far-infrared lines of [CII] and [OI](63um) and the TIR. The line maps ...
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Photoevaporation of the Jovian circumplanetary disk I. Explaining the orbit of Callisto and the lack of outer regular satellites
May, 2020
Context: The Galilean satellites are thought to have formed from a circumplanetary disk (CPD) surrounding Jupiter. When it reached a critical mass, Jupiter opened an annular gap in the solar protoplanetary disk (PPD) that might have exposed the CPD to radiation from the young Sun or from the st...
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