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Overview of the ESCAPE Dark Matter Test Science Project for astronomers. [PDF]
Open Res EurPearson J +3 more
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On the ambipolar diffusion formulation for ion-neutral drifts in the non-negligible drift velocity limit. [PDF]
Philos Trans A Math Phys Eng SciHillier AS.
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Stellar Jets and Bipolar Outflows
Astrophysics and Space Science Library, 1993L. Errico, A. Vittone
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, 2017 Young stars are usually associated with two types of high velocity phenomena: stellar jets and bipolar outflows. Jets (and their accompanying counter-jets) are highly collimated, have very high velocities in the range 100–1000 km s−1 and may extend out of the star-forming cores for distances as great as 10 pc.
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Stellar and galactic jets: theoretical issues
Canadian Journal of Physics, 1986 Theoretical issues pertaining to the modelling of jets in young stellar objects and in active galactic nuclei are reviewed. The strong morphological similarities between these two types of sources are emphasized, and observational constraints on the basic physical mechanisms that may be responsible for the jet phenomenon are outlined.
Arieh Königl
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The Kelvin-Helmholtz Instability in Stellar Jets
, 2009The Kelvin-Helmholtz Instability (KHI) is amongst the most relevant processes occurring in outflows propagating through an external medium. The KHI can critically affect the dynamics of jets leading to their disruption, but at same time it drives the formation of the peculiar morphologies observed in stellar collimated outflows.
E. Trussoni
semanticscholar +2 more sources
Measurement of Physical Conditions in Stellar Jets
, 2008This article summarizes the physics needed to interpret spectra of stellar jets, reviews the history of analysis techniques applied to these objects, discusses some recent results, and considers the prospects for future research in this area.
P. Hartigan
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Laboratory Experiments of Stellar Jets from the Perspective of an Observer
Astrophysics and Space Science, 2005Patrick Hartigan
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Astrophysics and Space Science, 2000
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Raga, A. C., Cantó, J., D'Alessio, P.
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zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Raga, A. C., Cantó, J., D'Alessio, P.
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Publications of the Astronomical Society of Australia, 1989
AbstractWe present maps in the visible emission lines of [S II] and the infrared emission lines of H2, at 2.12μm, for several bipolar outflow complexes which exhibit jet structures. A comparison of the morphology of this infrared emission and that seen in visible emission lines shows both the visible and the H2 emission exhibit clumpy structure on ...
W. J. Zealey +7 more
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AbstractWe present maps in the visible emission lines of [S II] and the infrared emission lines of H2, at 2.12μm, for several bipolar outflow complexes which exhibit jet structures. A comparison of the morphology of this infrared emission and that seen in visible emission lines shows both the visible and the H2 emission exhibit clumpy structure on ...
W. J. Zealey +7 more
openaire +1 more source