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F. F. S. van der Tak

Researcher at Netherlands Institute for Space Research

Publications -  325
Citations -  18198

F. F. S. van der Tak is an academic researcher from Netherlands Institute for Space Research. The author has contributed to research in topics: Star formation & Protostar. The author has an hindex of 63, co-authored 314 publications receiving 16781 citations. Previous affiliations of F. F. S. van der Tak include Kapteyn Astronomical Institute & National Institute for Space Research.

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Modeling the water line emission from the high-mass star-forming region AFGL2591

TL;DR: In this article, the authors investigate the diagnostic value of specific water transitions in high-mass star-forming regions, and find that the low-lying transitions of water are sensitive to outflow features, and represent the excitation conditions in outer regions.
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The role of planetary interior in the long-term evolution of atmospheric CO2on Earth-like exoplanets

TL;DR: In this article, the role of the thermal evolution of the planetary interior on the long-term carbon cycle of Earth-like exoplanets was investigated, in particular, the effects of radiogenic mantle heating, core size, and planetary mass on the atmospheric partial CO2 pressure.
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Infrared dark clouds on the far side of the Galaxy

TL;DR: In this paper, the authors used THz absorption spectroscopy to solve the distance ambiguity associated with kinematic distances for the IR-dark clouds in the TOP100 ATLASGAL sample, a flux-limited selection of massive clumps in different evolutionary phases of star formation.
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Chasing discs around O-type (proto)stars - ALMA evidence for an SiO disc and disc wind from G17.64+0.16

TL;DR: In this paper, the authors presented high angular resolution 0.2 arcsec continuum and molecular emission line Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of G17.64+0.16 in Band 6 (220GHz) taken as part of a campaign in search of circumstellar discs around (proto-O-stars).
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Multi-line Herschel/HIFI observations of water reveal infall motions and chemical segregation around high-mass protostars

TL;DR: In this paper, the authors used HIFI maps of the 987 GHz H2O 202-111 emission to measure the sizes and shapes of 19 high-mass protostellar envelopes.