F
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.
Papers
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Journal ArticleDOI
Spectrally resolved CII emission in M~33 ({\tt HerM33es}): Physical conditions and kinematics around BCLMP 691
J. Braine,Pierre Gratier,C. Kramer,Frank P. Israel,F. F. S. van der Tak,Bhaswati Mookerjea,M. Boquien,Fatemeh Tabatabaei,P. van der Werf,Carsten Henkel +9 more
TL;DR: In this article, high spectral resolution observations of the CII\ line at 158 µm were taken with the HIFI heterodyne spectrometer on the Herschel satellite, and the authors estimated the C$^+$ column density to be $N_{C^+} \approx 1.3 \times 10^{17} \cmt.
Journal ArticleDOI
Water abundances in high-mass protostellar envelopes: Herschel observations with HIFI
M. Marseille,F. F. S. van der Tak,Fabrice Herpin,Friedrich Wyrowski,L. Chavarria,Bastien Pietropaoli +5 more
TL;DR: In this article, the authors derived the dense core structure and the water abundance in four massive star-forming regions which may help understand the earliest stages of massive star formation using the Herschel-HIFI data.
Journal ArticleDOI
The evolution of young HII regions
P. D. Klaassen,Katharine G. Johnston,James Urquhart,Joseph C. Mottram,T. Peters,Rolf Kuiper,Henrik Beuther,F. F. S. van der Tak,Ciriaco Goddi +8 more
TL;DR: In this article, high-resolution ALMA observations of nine HII regions selected from the Red MSX Source (RMS) survey with compact radio emission and bolometric luminosities greater than 10$^4$ L$_\odot$ were presented.
Journal ArticleDOI
Probing the high-redshift universe with SPICA: Toward the epoch of reionisation and beyond
Eiichi Egami,Simona Gallerani,Raffaella Schneider,Andrea Pallottini,Livia Vallini,E. Sobacchi,Andrea Ferrara,Simone Bianchi,M. Bocchio,Stefania Marassi,Lee Armus,Luigi Spinoglio,Andrew Blain,M. Bradford,David L. Clements,Helmut Dannerbauer,Helmut Dannerbauer,J. A. Fernández-Ontiveros,J. A. Fernández-Ontiveros,Eduardo González-Alfonso,Matthew Joseph Griffin,Carlotta Gruppioni,Hidehiro Kaneda,Kotaro Kohno,S. C. Madden,Hideo Matsuhara,Francisco Najarro,Takao Nakagawa,S. J. Oliver,Kazuyuki Omukai,Takashi Onaka,Chris Pearson,Ismael Perez-Fournon,Ismael Perez-Fournon,Pablo G. Pérez-González,Pablo G. Pérez-González,Daniel Schaerer,Douglas Scott,Stephen Serjeant,J. D. Smith,F. F. S. van der Tak,F. F. S. van der Tak,Takehiko Wada,Hidenobu Yajima +43 more
TL;DR: In this article, the authors examined the feasibility and scientific potential of such observations with SPICA's far-infrared spectrometer SAFARI, which will probe a spectral range (35-230 μm) that will be unexplored by ALMA and JWST.
Journal ArticleDOI
The molecular gas mass of M 33
Pierre Gratier,Jonathan Braine,K. F. Schuster,Erik Rosolowsky,Médéric Boquien,D. Calzetti,Francoise Combes,C. Kramer,Carsten Henkel,Carsten Henkel,Fabrice Herpin,Frank P. Israel,Baerbel Koribalski,Bhaswati Mookerjea,Fatemeh Tabatabaei,Fatemeh Tabatabaei,Markus Röllig,F. F. S. van der Tak,F. F. S. van der Tak,P. van der Werf,Martina C. Wiedner +20 more
TL;DR: In this article, the authors used a sophisticated Bayesian formalism to derive the most likely values for each of the parameters mentioned above as a function of position in the nearby prototypical low metallicity (12 + log log O/H) ~ 8.4) spiral galaxy M 33.