[HTML][HTML] Jets from young stars
TP Ray, J Ferreira - New Astronomy Reviews, 2021 - Elsevier
Jets are ubiquitous in the Universe and are seen from a large number of astrophysical
objects including active galactic nuclei, gamma ray bursters, micro-quasars, proto-planetary …
objects including active galactic nuclei, gamma ray bursters, micro-quasars, proto-planetary …
Magnetically-driven jets from Keplerian accretion discs
J Ferreira - arXiv preprint astro-ph/9607057, 1996 - arxiv.org
Non-relativistic, magnetically-driven jets are constructed by taking self-consistently into
account the feedback on the underlying accretion disc. It is shown that such jets are mostly …
account the feedback on the underlying accretion disc. It is shown that such jets are mostly …
Herbig-haro objects
RD Schwartz - IN: Annual review of astronomy and astrophysics …, 1983 - adsabs.harvard.edu
Progress in the understanding of Herbig-Haro (HH) objects is reviewed. The results of
optical studies of the proper motions and alignments, variability, and polarization of HH …
optical studies of the proper motions and alignments, variability, and polarization of HH …
Stellar jets with intrinsically variable sources
AC Raga, J Cantó, L Binette… - … ), vol. 364, Dec. 1, 1990, p …, 1990 - adsabs.harvard.edu
Abstract Models for high Mach number, isothermal, pressure-matched jets ejected from
sources with variable velocities are presented. It is found that the relaxation of the …
sources with variable velocities are presented. It is found that the relaxation of the …
[HTML][HTML] Exact, algebraic solutions of the thin-shell two-wind interaction problem
J Canto, AC Raga, FP Wilkin - Astrophysical Journal v. 469, p …, 1996 - adsabs.harvard.edu
We have developed a formalism based on considerations of linear and angular momentum
conservation for solving axisymmetric, steady," thin-shell" problems, which is applicable to …
conservation for solving axisymmetric, steady," thin-shell" problems, which is applicable to …
Type I planetary nebulae
M Peimbert, S Torres-Peimbert - … -International Astronomical Union, 1983 - cambridge.org
The general properties of PN of Type I are reviewed. A list of 29 PN of Type I is presented,
most of them are bipolar. Their bipolar nature might be a direct consequence of the large …
most of them are bipolar. Their bipolar nature might be a direct consequence of the large …
The structure and evolution of radiatively cooling jets
JM Blondin, BA Fryxell, A Konigl - … Part 1 (ISSN 0004-637X), vol …, 1990 - adsabs.harvard.edu
The structure and evolution of radiatively cooling, supersonic jets are explored by means of
two-dimensional numerical simulations. The simulations reveal that the basic morphology of …
two-dimensional numerical simulations. The simulations reveal that the basic morphology of …
A Unified Model for Bipolar Outflows from Young Stars: Kinematic Signatures of Jets, Winds, and Their Magnetic Interplay with the Ambient Toroids
H Shang, CF Liu, R Krasnopolsky… - The Astrophysical …, 2023 - iopscience.iop.org
Kinematic signatures of the jet, winds, multicavities, and episodic shells arising in the unified
model of bipolar outflows developed in Shang et al.(Paper I), in which an outflow forms by …
model of bipolar outflows developed in Shang et al.(Paper I), in which an outflow forms by …
[HTML][HTML] Large proper motions of the Herbig-Haro objects HH 1 and HH 2
GH Herbig, BF Jones - Astronomical Journal, vol. 86, Aug. 1981 …, 1981 - adsabs.harvard.edu
Crossley and 120-in. direct plates obtained between 1946 and 1980 have been measured
for the proper motions of the Herbig-Haro objects HH 1, HH 2, and HH 3, which were then …
for the proper motions of the Herbig-Haro objects HH 1, HH 2, and HH 3, which were then …
On the nature of bipolar sources in dense molecular clouds
A Konigl - Astrophysical Journal, Part 1, vol. 261, Oct. 1, 1982, p …, 1982 - adsabs.harvard.edu
An attempt is made to present a unified interpretation of anisotropic emission and outflow
phenomena which are detected over a wide range of scales in the vicinity of young stellar …
phenomena which are detected over a wide range of scales in the vicinity of young stellar …