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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Herschel‐PACS observations of [O i]63 μm towards submillimetre galaxies at z ∼ 1
Kristen Coppin,A. L. R. Danielson,James E. Geach,Jacqueline Hodge,A. M. Swinbank,Julie Wardlow,Frank Bertoldi,A. D. Biggs,W. N. Brandt,Paola Caselli,Scott Chapman,Helmut Dannerbauer,James Dunlop,Thomas R. Greve,Fred Hamann,Rob Ivison,Rob Ivison,Alexander Karim,Kirsten Kraiberg Knudsen,Karl M. Menten,Eva Schinnerer,Ian Smail,Marco Spaans,Fabian Walter,Tracy Webb,P. van der Werf +25 more
TL;DR: In this paper, the authors used PACS spectroscopy of the [O I]63 μm far-infrared cooling line from a sample of six unlensed and spectroscopically confirmed 870 μm selected submillimetre (submm) galaxies (SMGs) at 1.1 < z < 1.6 from the LABOCA Extended Chandra Deep Field South (ECDFS) Submm Survey (LESS).
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CO line emission in the halo of a radio galaxy at z=2.6
Nicole P. H. Nesvadba,Nicole P. H. Nesvadba,Roberto Neri,C. De Breuck,Matthew D. Lehnert,D. Downes,Fabian Walter,Alain Omont,Francois Boulanger,Nick Seymour +9 more
TL;DR: In this paper, the authors reported the detection of luminous CO(3-2) line emission in the halo of the z=2.6 radio galaxy TXS0828+193, which has no detected counterpart at optical to mid-infrared wavelengths implying a stellar mass < few x10^9 M_sun and relatively low star-formation rates.
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Ultraviolet Observations of the Powering Source of the Supergiant Shell in IC 2574
S. G. Stewart,Fabian Walter +1 more
TL;DR: In this paper, a multiband analysis of the region containing the supergiant H I shell in the nearby dwarf irregular galaxy IC 2574 presents evidence of a causal relationship between a central star cluster, the surrounding expanding H I shells, and secondary star formation sites on the rim of the shell.
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Towards A Removal of Temperature Dependencies from Abundance Determinations
Kevin V. Croxall,Jd Smith,Bernhard R. Brandl,Brent Groves,Robert C. Kennicutt,K. Kreckel,B. D. Johnson,Eric W. Pellegrini,Karin Sandstrom,Fabian Walter,L. Armus,P. Beirao,D. Calzetti,Daniel A. Dale,Maud Galametz,J. L. Hinz,L. K. Hunt,Jin Koda,Eva Schinnerer +18 more
TL;DR: In this article, the authors used the [O III] 88 \micron\ fine-structure line in NGC 628 that were obtained as part of the KINGFISH program to derive oxygen abundances for seven HII regions.
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Dark and luminous matter in THINGS dwarf galaxies
TL;DR: In this paper, mass models for the dark matter component of seven dwarf galaxies taken from "The HI Nearby Galaxy Survey" (THINGS) and compare these with those from numerical Lambda Cold Dark Matter (LCDM) simulations are presented.