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
Infrared dark clouds on the far side of the Galaxy
Andrea Giannetti,Friedrich Wyrowski,Silvia Leurini,James Urquhart,Timea Csengeri,Karl M. Menten,Leonardo Bronfman,F. F. S. van der Tak +7 more
TL;DR: In this article, 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.
Journal ArticleDOI
SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
J. A. Fernández-Ontiveros,Lee Armus,Maarten Baes,Jeronimo Bernard-Salas,Alberto D. Bolatto,Jonathan Braine,Laure Ciesla,I. De Looze,Eiichi Egami,J. Fischer,M. Giard,Eduardo González-Alfonso,Gian Luigi Granato,Carlotta Gruppioni,Masatoshi Imanishi,Daisuke Ishihara,Hidehiro Kaneda,S. C. Madden,Matthew A. Malkan,H. Matsuhara,Mikako Matsuura,Tohru Nagao,Francisco Najarro,Takao Nakagawa,Takashi Onaka,Shinki Oyabu,Miguel Pereira-Santaella,I. Perez Fournon,I. Perez Fournon,Peter Roelfsema,Paola Santini,L. Silva,J. D. T. Smith,L. Spinoglio,F. F. S. van der Tak,Takehiko Wada,Ronin Wu +36 more
TL;DR: In this paper, the authors investigated how SPICA observations could be exploited to understand key aspects in the chemical evolution of galaxies: the assembly of nearby galaxies based on the spatial distribution of heavy element abundances, the global content of metals in galaxies reaching the knee of the luminosity function up to $z \sim 3$, and the dust composition of galaxies at high-$z$.
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The Herschel-HIFI view of mid-IR quiet massive protostellar objects
Fabrice Herpin,L. Chavarria,T. Jacq,J. Braine,F. F. S. van der Tak,Friedrich Wyrowski,E. F. van Dishoeck,A. Baudry,Sylvain Bontemps,Lars E. Kristensen,M. Schmalzl,J. Mata +11 more
TL;DR: In this paper, the authors present Herschel/HIFI observations (WISH KP) of 14 water lines in a small sample of galactic massive protostellar objects: NGC6334I(N), DR21(OH), IRAS16272-4837, and IRAS05358+3543.
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Low noise MgB2 hot electron bolometer mixer operated at 5.3 THz and at 20 K
Yuner Gan,Yuner Gan,B. Mirzaei,B. Mirzaei,J. R.G. Silva,J. R.G. Silva,Jin Chang,Serguei Cherednichenko,F. F. S. van der Tak,F. F. S. van der Tak,J. R. Gao,J. R. Gao +11 more
TL;DR: In this paper, a superconducting MgB2 hot electron bolometer (HEB) mixer working at the frequency of 5.3 GHz with 20 K operation temperature was demonstrated.
Journal ArticleDOI
Exploring the formation pathways of formamide - Near young O-type stars
V. Allen,V. Allen,F. F. S. van der Tak,Ana López-Sepulcre,Álvaro Sánchez-Monge,Victor M. Rivilla,Riccardo Cesaroni +6 more
TL;DR: In this paper, the authors examined high angular resolution (0.2″) Atacama Large Millimeter/submillimeter Array maps of six sources in three high-mass star-forming regions and compared the spatial extent, integrated emission peak position, and velocity structure of HNCO and H2 CO line emission with that of NH2 CHO through spectral modeling.