J. Eislöffel
Max Planck Society
23 Papers
141 Citations
J. Eislöffel is an academic researcher from Max Planck Society. The author has contributed to research in topics: Stars & Jet (fluid). The author has an hindex of 8, co-authored 23 publications.
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Papers
Jets and Outflows From Star to Cloud: Observations Confront Theory
Alejandro Frank,Thomas P. Ray,S. Cabrit,Patrick Hartigan,Héctor G. Arce,Francesca Bacciotti,John Bally,Myriam Benisty,J. Eislöffel,Manuel Güdel,Sergey Lebedev,Brunella Nisini,Alejandro C. Raga +12 more
TL;DR: In this article, the role of jets and outflows in star and planet formation is reviewed and a review of jet/outflow phenomena is organized into three length-scale domains: Source and Disk Scales, Envelope Scales and Parent Cloud Scales where global momentum injection into cluster/cloud environments become relevant.
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Jets and Outflows from Star to Cloud: Observations Confront Theory
Alejandro Frank,Thomas P. Ray,S. Cabrit,Patrick Hartigan,Héctor G. Arce,Francesca Bacciotti,John Bally,Myriam Benisty,J. Eislöffel,Manuel Güdel,Sergey Lebedev,Brunella Nisini,Alejandro C. Raga +12 more
- 14 Feb 2014
TL;DR: In this paper, the role of jets and outflows in star and planet formation is reviewed and a review of jet/outflow phenomena is organized into three length-scale domains: Source and Disk Scales, Envelope Scales and Parent Cloud Scales where global momentum injection into cluster/cloud environments become relevant.
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Physical properties of the jet from DG Tauri on sub-arcsecond scales with HST/STIS
L. Maurri,Francesca Bacciotti,Linda Podio,J. Eislöffel,Thomas P. Ray,Reinhard Mundt,Ugo Locatelli,Deirdre Coffey +7 more
TL;DR: In this paper, the authors derived the physical properties at the base of the jet from DG Tau both along and across the flow and as a function of velocity, and demonstrated that the derived properties of the DG Tau jet are consistent with magneto-centrifugal theory.
Infrared observations of the flaring maser source G358.93-0.03 : SOFIA confirms an accretion burst from a massive young stellar object
Bringfried Stecklum,V. Wolf,Hendrik Linz,A. Caratti o Garatti,S. Schmidl,Sylvio Klose,J. Eislöffel,C. Fischer,Crystal L. Brogan,Ross A. Burns,O. Bayandina,Claudia Cyganowski,Mark Gurwell,Todd R. Hunter,Naomi Hirano,Kee-Tae Kim,G. C. MacLeod,G. C. MacLeod,Karl M. Menten,M. Olech,Gabor Orosz,Andrej M. Sobolev,T. K. Sridharan,Gabriele Surcis,Koichiro Sugiyama,J.L. Van der Walt,A. E. Volvach,Yoshinori Yonekura +27 more
TL;DR: In this paper, the authors performed near-infrared (NIR) and farinfrared observations to prove or disprove whether the 6.7 GHz CH3 OH maser flare was driven by an accretion burst.
An Optical/Infrared Outburst in the Exciting Source of HH 7–11
J. Eislöffel,E. Günther,F. V. Hessman,Reinhard Mundt,R. Poetzel,J. S. Carr,Steven V. W. Beckwith,Tom Ray +7 more
- 01 Jan 1993
TL;DR: In this article, the authors reported an outburst of SVS 13, the exciting source of the HH 7-11 outflow, in the optical and near-infrared wavelength region (see also Eisloffel et al., 1991).
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