O
Oliver Krause
Researcher at Max Planck Society
Publications - 165
Citations - 14831
Oliver Krause is an academic researcher from Max Planck Society. The author has contributed to research in topics: Star formation & Galaxy. The author has an hindex of 48, co-authored 162 publications receiving 13695 citations. Previous affiliations of Oliver Krause include University of Arizona.
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Journal ArticleDOI
From high-mass starless cores to high-mass protostellar objects
Henrik Beuther,Th. Henning,Hendrik Linz,Oliver Krause,Markus Nielbock,Juergen Steinacker,Juergen Steinacker +6 more
TL;DR: In this article, the spectral and physical evolution of high-mass star formation from the earliest evolutionary stage of starless cores, via highmass cores with embedded low-to intermediate-mass objects, to finally highmass protostellar objects is studied.
Journal ArticleDOI
Enhanced dust heating in the bulges of early-type spiral galaxies
Charles W. Engelbracht,Leslie K. Hunt,Ramin A. Skibba,Joannah L. Hinz,D. Calzetti,Karl D. Gordon,H. Roussel,Alison F. Crocker,Karl Misselt,Alberto D. Bolatto,Robert C. Kennicutt,P. N. Appleton,Lee Armus,P. Beirão,Bernhard R. Brandl,Kevin V. Croxall,Daniel A. Dale,Bruce T. Draine,G. Dumas,A. Gil de Paz,Brent Groves,Cai-Na Hao,Benjamin D. Johnson,Jin Koda,Oliver Krause,Adam K. Leroy,Sharon E. Meidt,Eric J. Murphy,Nurur Rahman,H. W. Rix,Karin Sandstrom,Marc Sauvage,Eva Schinnerer,J. D. T. Smith,Sundar Srinivasan,L. Vigroux,Fabian Walter,B. E. Warren,Christine D. Wilson,Mark G. Wolfire,Stefano Zibetti +40 more
TL;DR: In this paper, the authors investigated the differences between the central 3 kpc and disk of 13 nearby galaxies by fitting models to measurements between 70 and 500 μm and found a significant temperature gradient in the cool dust component in all galaxies, with a mean centerto-disk temperature ratio of 1.15 ± 0.03.
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A study of heating and cooling of the ism in ngc 1097 with herschel-pacs and spitzer-irs
P. Beirao,Lee Armus,George Helou,P. N. Appleton,J. D. T. Smith,Kevin V. Croxall,Eric J. Murphy,Daniel A. Dale,Bruce T. Draine,Mark G. Wolfire,Karin Sandstrom,G. Aniano,Alberto D. Bolatto,Brent Groves,Bernhard R. Brandl,Eva Schinnerer,Alison F. Crocker,Joannah L. Hinz,H.-W. Rix,Robert C. Kennicutt,Daniela Calzetti,A. Gil de Paz,Gaelle Dumas,Maud Galametz,Karl D. Gordon,Cai-Na Hao,Benjamin D. Johnson,Jin Koda,Oliver Krause,T. P. R. van der Laan,Adam K. Leroy,Yiming Li,Sharon E. Meidt,Jennifer Donovan Meyer,Nurur Rahman,Helene Roussel,Marc Sauvage,Sundar Srinivasan,L. Vigroux,Fabian Walter,B. E. Warren +40 more
TL;DR: In this paper, a detailed study of the spatial variation of the far-infrared (FIR) [C II]158 μm and [O I]63 μm lines and midinfrared H2 emission lines as tracers of gas cooling, and of the polycyclic aromatic hydrocarbon (PAH) bands as tracer of the photoelectric heating, using Herschel-PACS and Spitzer-IRS infrared spectral maps.
Journal ArticleDOI
The ISOPHOT 170 μm Serendipity Survey II. The catalog of optically identified galaxies
TL;DR: The ISOPHOT Serendipity Sky Survey strip-scanning measurements covering 15% of the far-infrared (FIR) sky at 170μm were searched for compact sources associated with optically identified galaxies.
Journal ArticleDOI
KINGFISH -- Key Insights on Nearby Galaxies: A Far-Infrared Survey with Herschel: Survey Description and Image Atlas
Robert C. Kennicutt,Daniela Calzetti,G. Aniano,P. N. Appleton,Lee Armus,P. Beirao,Alberto D. Bolatto,Bernhard R. Brandl,Alison F. Crocker,Kevin V. Croxall,Daniel A. Dale,J. Dononvan Meyer,Bruce T. Draine,Charles W. Engelbracht,Maud Galametz,Karl D. Gordon,Brent Groves,Cai-Na Hao,George Helou,J. L. Hinz,Leslie K. Hunt,Benjamin D. Johnson,Jin Koda,Oliver Krause,Adam K. Leroy,Yongbao Li,Sharon E. Meidt,E. Montiel,Eric J. Murphy,Nurur Rahman,H-W. Rix,Helene Roussel,Karin Sandstrom,Marc Sauvage,Eva Schinnerer,Ramin A. Skibba,J. D. T. Smith,Sundar Srinivasan,L. Vigroux,Frederick M. Walter,C. D. Wilson,Mark G. Wolfire,Stefano Zibetti +42 more
TL;DR: The Kingfish project (Key Insights on Nearby Galaxies: a Far-Infrared Survey with Herschel) as discussed by the authors is an imaging and spectroscopic survey of 61 nearby galaxies, chosen to cover a wide range of galaxy properties and local interstellar medium (ISM) environments found in the nearby Universe.