• Corpus ID: 18805208

A MODEL FOR THE CROSS SECTION OF A TURBULENT, RADIATIVE JET OR WAKE

@article{Cant2003AMF,
  title={A MODEL FOR THE CROSS SECTION OF A TURBULENT, RADIATIVE JET OR WAKE},
  author={J. Cant{\'o} and Alejandro C. Raga and Angels Riera},
  journal={Revista Mexicana De Astronomia Y Astrofisica},
  year={2003},
  volume={39},
  pages={207-212}
}
Resumen en: We present an analytical model for the cross section of a turbulent, radiative jet or wake. This model is appropriate for modeling HH jets, or “wakes” l... 

Figures and Tables from this paper

3-D kinematics of the HH 110 jet
We present new results on the kinematics of the jet HH 110. New proper motion measurements have been calculated from [SII] CCD images obtained with a time baseline of nearly fifteen years. HH 110
On an Azimuthally Symmetric Theory of Gravitation II Outflows as a Gravitational Phenomena
This is a second reading on the Azimuthally Symmetric Theory of Gravitation (ASTG) set-out in Nyambuya (2009). This theory is built on Poisson’s well known equation and it has been shown there-in
High-mass star formation at sub-50 au scales
Context. The hierarchical process of star formation has so far mostly been studied on scales from thousands of au to parsecs, but the smaller sub-1000 au scales of high-mass star formation are still