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
More filters
Journal ArticleDOI
Molecular Gas in M82: Resolving the Outflow and Streamers
TL;DR: In this paper, a high-resolution (36, 70 pc) 12CO (J = 1 → 0) mosaic of the molecular gas in M82 covering an area of 25 × 35 (2.8 × 3.9 kpc) obtained with the Owens Valley Radio Observatory millimeter interferometer.
Journal ArticleDOI
Molecular gas in the host galaxy of a quasar at redshift z = 6.42
Fabian Walter,Frank Bertoldi,Chris Carilli,Pierre Cox,K. Y. Lo,Roberto Neri,Xiaohui Fan,A. Omont,A. Omont,Michael A. Strauss,Karl M. Menten +10 more
TL;DR: The presence of about 2 × 1010 M[circdot] of H2 in an object at this time demonstrates that molecular gas enriched with heavy elements can be generated rapidly in the youngest galaxies.
Journal ArticleDOI
On the effect of the Cosmic Microwave Background in high-redshift (sub-)millimeter observations
Elisabete da Cunha,Brent Groves,Fabian Walter,Roberto Decarli,Axel Weiss,Chris Carilli,Emanuele Daddi,David Elbaz,Rob Ivison,Roberto Maiolino,Dominik Riechers,Hans-Walter Rix,Mark Sargent,Ian Smail +13 more
TL;DR: In this paper, the impact of the warmer cosmic microwave background (CMB) on (sub-)millimeter observations of high-redshift galaxies is discussed and the spectral energy distribution model is proposed.
Journal ArticleDOI
High-Resolution Dark Matter Density Profiles of THINGS Dwarf Galaxies: Correcting for Noncircular Motions
TL;DR: In this paper, a new method was proposed to remove the impact of random and small-scale noncircular motions from H I velocity fields in (dwarf) galaxies in order to better constrain the dark matter properties for these objects.
Journal ArticleDOI
ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass
Rychard Bouwens,Manuel Aravena,Roberto Decarli,Fabian Walter,Fabian Walter,Elisabete da Cunha,Elisabete da Cunha,Ivo Labbé,Franz E. Bauer,Franz E. Bauer,Franz E. Bauer,Frank Bertoldi,Chris Carilli,Scott Chapman,Emanuele Daddi,Jacqueline Hodge,Rob Ivison,Rob Ivison,Alex Karim,Olivier Le Fevre,Benjamin Magnelli,Kazuaki Ota,Dominik Riechers,Ian Smail,Paul van der Werf,Axel Weiss,Pierre Cox,David Elbaz,Jorge González-López,Leopoldo Infante,Pascal Oesch,Jeff Wagg,S. Wilkins +32 more
TL;DR: In this paper, the authors make use of deep 1.2 mm continuum observations (12.7 μJy beam−1 rms) of a 1 arcmin² region in the Hubble Ultra Deep Field to probe dust-enshrouded star formation from 330 Lyman-break galaxies spanning the redshift range z = 2−10 (to ∼2-3 M⊙ yr−1 at 1σ over the entire range).