M
Michiel R. Hogerheijde
Researcher at University of Amsterdam
Publications - 201
Citations - 9781
Michiel R. Hogerheijde is an academic researcher from University of Amsterdam. The author has contributed to research in topics: Protostar & Young stellar object. The author has an hindex of 59, co-authored 201 publications receiving 9054 citations. Previous affiliations of Michiel R. Hogerheijde include University of Arizona & Steward Health Care System.
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Journal ArticleDOI
Water in star-forming regions with Herschel (WISH). II. Evolution of 557 GHz 110-101 emission in low-mass protostars
Lars E. Kristensen,E. F. van Dishoeck,Edwin Bergin,Ruud Visser,Umut A. Yildiz,I. San Jose-Garcia,Jes K. Jørgensen,Gregory J. Herczeg,Doug Johnstone,Doug Johnstone,S. F. Wampfler,Arnold O. Benz,Simon Bruderer,Sylvie Cabrit,Paola Caselli,Paola Caselli,Steven D. Doty,Daniel Harsono,Fabrice Herpin,Michiel R. Hogerheijde,Agata Karska,T. A. van Kempen,René Liseau,Brunella Nisini,Mario Tafalla,F. F. S. van der Tak,Friedrich Wyrowski +26 more
TL;DR: In this paper, the first systematic survey of spectrally resolved water emission in 29 low-mass (L 10 km s−1) star-forming regions has been published.
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LIME - a flexible, non-LTE line excitation and radiation transfer method for millimeter and far-infrared wavelengths
TL;DR: In this article, the authors present a new code for solving the molecular and atomic excitation and radiation transfer problem in a molecular gas and predicting emergent spectra. This code works in arbitrary three dimensional geometry using unstructured Delaunay latices for the transport of photons.
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Envelope structure on 700 AU scales and the molecular outflows of low-mass young stellar objects
TL;DR: Trends support the hypothesis that outflows are driven by accretion through a disk, with a global mass infall rate determined by the mass and density of the envelope.
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Gas and Dust Emission at the Outer Edge of Protoplanetary Disks
TL;DR: In this article, the authors investigate the apparent discrepancy between gas and dust outer radii derived from millimeter observations of protoplanetary disks and show that the outer radius derived from the dust continuum emission is always significantly smaller than the extent of the molecular gas disk traced by CO emission.
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Empirical constraints on turbulence in protoplanetary accretion disks
TL;DR: In this paper, the authors present arcsecond-scale Submillimeter Array observations of the CO(3-2) line emission from the disks around the young stars HD 163296 and TW Hya at a spectral resolution of 44m − 1.