F
Fabian Walter
Researcher at Max Planck Society
Publications - 1053
Citations - 92179
Fabian Walter is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 146, co-authored 999 publications receiving 83016 citations. Previous affiliations of Fabian Walter include California Institute of Technology & University of Bonn.
Papers
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Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: The KINGFISH Sample
G. Aniano,G. Aniano,B. T. Draine,Leslie K. Hunt,Karin Sandstrom,Daniela Calzetti,R. C. Kennicutt,R. C. Kennicutt,Daniel A. Dale,Maud Galametz,Karl D. Gordon,Adam K. Leroy,J. D. T. Smith,Helene Roussel,Marc Sauvage,Fabian Walter,Lee Armus,Alberto D. Bolatto,Médéric Boquien,Alison F. Crocker,I. De Looze,I. De Looze,J. Donovan Meyer,George Helou,J. Hinz,Benjamin D. Johnson,Jin Koda,Adam Miller,Adam Miller,E. Montiel,E. Montiel,Eric J. Murphy,M. Relaño,H.-W. Rix,Eva Schinnerer,Ramin A. Skibba,Mark G. Wolfire,Charles W. Engelbracht +37 more
TL;DR: In this paper, the Kingfish project galaxies were modeled with data from 3.6 micron to 500 micron, and the authors provided well-resolved maps for the dust properties.
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Resolving the Radio Emission from the Quasar P172+18 at $z = 6.82$
TL;DR: In this paper, the authors presented high angular resolution imaging of the quasar PSO J172.7734 at 1.53 GHz with the Very Long Baseline Array (VLBA).
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Faint co line wings in four star-forming (ultra)luminous infrared galaxies
Adam K. Leroy,Fabian Walter,Roberto Decarli,Alberto D. Bolatto,Laura K. Zschaechner,Axel Weiss +5 more
TL;DR: In this article, the authors reported the results of a search for large velocity width, low-intensity line wings, a commonly used signature of molecular outflows, in four low redshift (ultra)luminous infrared galaxies that appear to be dominated by star formation.
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Rosat x-ray observations of the dwarf galaxy holmberg ii
TL;DR: In this paper, a study of the irregular dwarf galaxy Holmberg II based on ROSAT Position Sensitive Proportional Counter observations (total exposure time: 22 ks) is presented, where X-ray emission from point sources as well as for diffuse emission, down to the detection limit of the ROSAT data.
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High resolution observations of a starburst at z = 0.223: resolved CO(1–0) structure
Francoise Combes,Santiago García-Burillo,Jonathan Braine,Eva Schinnerer,Fabian Walter,Luis Colina,Maryvonne Gerin +6 more
TL;DR: In this paper, the results of CO(1-0) emission mapping with the IRAM interferometer, at 1 arcsec, resolution, of the z=0.223 ultra-luminous starburst IRAS 11582+3020.