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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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Journal ArticleDOI

Origin of hydrogen fluoride emission in the Orion Bar An excellent tracer for CO-dark H-2 gas clouds

U. Kavak, +6 more
- 01 Nov 2019 - 
TL;DR: In this article, the authors used a Herschel/HIFI strip map of the hydrogen fluoride (HF) column density map to understand the origin of HF emission in the Orion Bar by comparing its spatial distribution with other tracers.
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Distribution of water in the G327.3-0.6 massive star-forming region

Silvia Leurini, +7 more
- 01 Jun 2017 - 
TL;DR: In this paper, the authors investigated the large-scale distribution of water in the G327.6 massive star-forming region and investigated possible variations of the water abundance as a function of evolution.
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The massive protostar W43-MM1 as seen by Herschel-HIFI water spectra: high turbulence and accretion luminosity

Fabrice Herpin, +9 more
- 02 Apr 2012 - 
TL;DR: In this article, the authors analyzed the gas dynamics from the line profiles using Herschel-HIFI observations of fourteen water lines in W43-MM1, a massive protostellar object in the luminous star cluster-forming region W43.
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A search for radio jets from massive young stellar objects. Association of radio jets with H2O and CH3OH masers

U. Kavak, +7 more
- 30 Nov 2020 - 
TL;DR: In this article, the authors used the Karl G. Jansky Very Large Array (VLA) to observe 18 high-mass star-forming regions in the C band and K band (1.3 cm, 0.3 arcsec resolution).
Journal ArticleDOI

Origin of hydrogen fluoride emission in the Orion Bar: An excellent tracer for CO-dark H2 gas clouds

U. Kavak, +3 more
- 01 Oct 2019 - 
TL;DR: In this paper, the authors examined three mechanisms to explain the hydrogen fluoride (HF) emission toward the Orion Bar, which is an interface between the ionized region around the Orion Trapezium stars and the Orion molecular cloud.