Results 251 to 260 of about 35,594 (296)

Cylindrical compression of thin wires by irradiation with a Joule-class short-pulse laser. [PDF]

Nat Commun
Laso Garcia A, Yang L, Bouffetier V, Appel K, Baehtz C, Hagemann J, Höppner H, Humphries O, Kluge T, Mishchenko M, Nakatsutsumi M, Pelka A, Preston TR, Randolph L, Zastrau U, Cowan TE, Huang L, Toncian T.   +17 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 Sci
Hillier AS.
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Outstanding Questions and Future Research on Magnetic Reconnection. [PDF]

Space Sci Rev
Nakamura R, Burch JL, Birn J, Chen LJ, Graham DB, Guo F, Hwang KJ, Ji H, Khotyaintsev YV, Liu YH, Oka M, Payne D, Sitnov MI, Swisdak M, Zenitani S, Drake JF, Fuselier SA, Genestreti KJ, Gershman DJ, Hasegawa H, Hoshino M, Norgren C, Shay MA, Shuster JR, Stawarz JE.   +24 more
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Tracing chemical depletion in evolved binaries hosting second-generation transition discs. [PDF]

Mon Not R Astron Soc
Mohorian M, Kamath D, Menon M, Amarsi AM, Van Winckel H, Fava C, Andrych K.   +6 more
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Saturn's F ring is intermittently shepherded by Prometheus. [PDF]

Sci Adv
Cuzzi JN, Marouf EA, French RG, Murray CD, Cooper NJ.   +4 more
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Relativistic jets from stellar black holes

, 2005
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The Dynamics of Stellar Jets

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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Stellar Outflows and Jets

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, R. Mundt, T. P. Ray, G. Sandell, T. Geballe, K. N. R. Taylor, P. M. Williams, H. Zinnecker   +7 more
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Properties of Knots in Cooling Stellar Jets

Astrophysics and Space Science, 2004
Modelling the formation of the maximal emission regions in Herbig-Haro flows, the socalled ‘knots,’ remains a main challenge in the investigation of the YSO’s outflows. Recent HST images of optical regions reveal their wide morphological variety. Knotty structures and arc-like regions coexist, suggesting that several mechanisms could be responsible for
RUBINI, FRANCESCO MARIO, C. Giovanardi, S. Lorusso, F. Leeuwin, F. Bacciotti   +4 more
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Coupled Stellar Jet/Molecular Outflow Models

Astrophysics and Space Science, 1994
Molecular outflows can be modelled as environmental material entrained into high velocity stellar jets. Even though models of this entrainment process are at this time quite uncertain, a few preliminary theoretical efforts have been made. Three different models are discussed, in which the molecular outflows are identified with the turbulent mixing ...
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