Laboratory studies of astrophysical jets

A Ciardi - Jets from Young Stars IV: From Models to Observations …, 2009 - Springer
Jets and outflows produced during star-formation are observed on many scales: from the
“micro-jets” which extend over a few hundred Astronomical Units to the “super-jets” which …

The Time Evolution of the HH 1 Jet Modeled as a Variable Outflow

A Castellanos-Ramírez, AC Raga… - The Astrophysical …, 2018 - iopscience.iop.org
The HH 1 jet is a chain of knots extending out to∼ 20''from the VLA 1 source of the HH 1/2
system. Four epochs of [S ii] images obtained with the Hubble Space Telescope over a∼ 20 …

An intepretive ballistic model for quasi-symmetric bipolar jet systems

AC Raga, A Noriega-Crespo… - Revista mexicana de …, 2011 - scielo.org.mx
Presentamos un modelo analítico, balístico para sistemas de chorros/contrachorros cuasi–
simetricos, considerando tanto el caso no relativista como el relativista. El modelo considera …

Tomographic Reconstruction of the Three-dimensional Structure of the HH30 Jet

F De Colle, C del Burgo, AC Raga - The Astrophysical Journal, 2010 - iopscience.iop.org
The physical parameters of Herbig–Haro (HH) jets are usually determined from emission-
line ratios, obtained from spectroscopy or narrowband imaging, assuming that the emitting …

On the time variability of the HH jet ejection process

F De Colle - Proceedings of the International Astronomical Union, 2010 - cambridge.org
Two-dimensional emission line images of the HH30 jet were recently used (De Colle et al.
2010) to recover the three-dimensional structure of the jet by applying standard tomographic …

[PS][PS] QUASI-SYMMETRIC BIPOLAR JETS 295

P Hartigan, JA Morse, B Reipurth, S Heathcote - astroscu.unam.mx
Murphy (2008). The magnetospheric magnetic field could have time-dependencies on
timescales similar to the solar cycle (ie, with periods~ 20 yr). From the observational point of …

[PS][PS] THE KINEMATICS AND VELOCITY ELLIPSOID OF THE G III STARS

OFNA NEBULA - 2011 - astroscu.unam.mx
To study the kinematics of the G giant stars (luminosity class III) use is made of proper
motions and parallaxes taken from van Leeuwen's new reduction of the Hipparcos catalog …