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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Kinematic and thermal structure at the onset of high-mass star formation
S. Bihr,Henrik Beuther,Hendrik Linz,Sarah Ragan,Martin Hennemann,J. Tackenberg,Rowan J. Smith,Oliver Krause,Thomas Henning +8 more
TL;DR: In this paper, the NH3 (1, 1) and (2, 2) lines within six very young high-mass star-forming regions comprised of infrared dark clouds (IRDCs), along with ISO-selected far-infrared emission sources (ISOSS) with the Karl G. Jansky Very Large Array (VLA) and the Effelsberg 100 m Telescope.
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A very young star forming region detected by the ISOPHOT Serendipity Survey
TL;DR: In this paper, the authors presented a multi-wavelength study of the star forming region ISOSS J 20298+3559, which was identified by a cross-correlation of cold compact sources from the 170 μ m ISOPHOT Serendipity Survey (ISOSS) database coinciding with objects detected by the MSX, 2MASS and IRAS infrared surveys.
PACS and SPIRE mapping of the enigmatic outflow source UYSO 1
Hendrik Linz,Oliver Krause,Henrik Beuther,Randolf Klein,B. Stecklum,Juergen Steinacker,A. M. Stutz +6 more
TL;DR: In this paper, the spectral energy peak of a star-forming core UYSO 1 has been observed to be at the interface between the hot H ii region Sh 2-297 and the cold dark nebula LDN 1657A, and the data identify cooler compact far-infrared sources of just a few solar masses hidden in this neighbouring dark cloud.
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Very cold and massive cores near ISOSS J18364-0221: Implications for the initial conditions of high-mass star-formation
TL;DR: In this paper, the authors reported the discovery of two very cold and massive molecular cloud cores in the region ISOSS J18364-0221 by a systematic search for very early evolutionary stages of high-mass stars using the 170 micron ISOPHOT Serendipity Survey (ISOSS).
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Star formation in the Cepheus Flare region: Implications from morphology and infrared properties of optically selected clouds
TL;DR: In this paper, a complex study of visual and infrared properties of ISM and an examination of cloud morphology was carried out using USNO, 2MASS, DIRBE, IRAS, and ISO data of an extended region in Cepheus to explore the conditions of cloud and star formation.