# Radiative Signatures of Parsec-Scale Magnetised Jets

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## Abstract

**:**

## 1. Introduction

## 2. Methods

#### 2.1. SRMHD Simulations

#### 2.2. Radiative Transfer Calculations and Synthetic Imaging

## 3. Results

## 4. Discussion and Conclusions

## Acknowledgments

## Author Contributions

## Conflicts of Interest

## References

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1. | Dashed values indicate the co-moving system. |

2. |

**Figure 1.**2D distribution of the pressure (

**left panel**) and magnetisation (

**right panel**) for different initial magnetisations (for details see text).

**Figure 2.**Radio maps (15 GHz) using the Very Long Baseline Array (VLBA) as the observing array for different initial magnetisations (indicated in top left corner). The convolving beam of $1.12\phantom{\rule{0.166667em}{0ex}}\mathrm{mas}\times 0.57\phantom{\rule{0.166667em}{0ex}}\mathrm{mas}$ is plotted in the lower right corner.

**Table 1.**Initial parameters for the special-relativistic magneto-hydrodynamical (SRMHD) in code units (varying values in bold face).

${\mathit{r}}_{\mathbf{m}}$ | ${\mathit{r}}_{\mathbf{j}}$ | ${\mathit{b}}_{\mathbf{m}}$ | ${\mathit{\beta}}_{\mathbf{m}}$ | $\mathit{\chi}$ | ${\Gamma}_{0}$ | ${\mathit{\rho}}_{\mathbf{a}}$ | $\mathit{\eta}$ | $\mathit{\kappa}$ | $\widehat{\mathit{\gamma}}$ | ${\mathit{\sigma}}_{0}$ |
---|---|---|---|---|---|---|---|---|---|---|

0.37 | 1.0 | 0.14 | 1.85 | 0.95 | 8.0 | 1.0 | 0.01 | 1.0 | 13/9 | 0.5 |

0.37 | 1.0 | 0.19 | 1.00 | 0.95 | 8.0 | 1.0 | 0.01 | 1.0 | 13/9 | 1.0 |

0.37 | 1.0 | 0.34 | 0.30 | 0.95 | 8.0 | 1.0 | 0.01 | 1.0 | 13/9 | 5.0 |

$\mathit{\vartheta}$ | ${\mathit{\u03f5}}_{\mathbf{e}}$ | ${\mathit{\u03f5}}_{\mathit{\gamma}}$ | ${\mathit{\zeta}}_{\mathbf{e}}$ | s | z | ${\mathit{\rho}}_{\mathbf{a}}$ | ${\mathit{R}}_{\mathbf{j}}$ |
---|---|---|---|---|---|---|---|

5${}^{\circ}$ | 0.3 | ${10}^{3}$ | 1.0 | 2.2 | 1.0 | $1.0\times {10}^{-23}\phantom{\rule{0.166667em}{0ex}}\mathrm{g}\phantom{\rule{0.166667em}{0ex}}{\mathrm{cm}}^{-3}$ | $3.0\times {10}^{18}\phantom{\rule{0.166667em}{0ex}}\mathrm{cm}$ |

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## Share and Cite

**MDPI and ACS Style**

Fromm, C.M.; Porth, O.; Younsi, Z.; Mizuno, Y.; De Laurentis, M.; Olivares, H.; Rezzolla, L.
Radiative Signatures of Parsec-Scale Magnetised Jets. *Galaxies* **2017**, *5*, 73.
https://doi.org/10.3390/galaxies5040073

**AMA Style**

Fromm CM, Porth O, Younsi Z, Mizuno Y, De Laurentis M, Olivares H, Rezzolla L.
Radiative Signatures of Parsec-Scale Magnetised Jets. *Galaxies*. 2017; 5(4):73.
https://doi.org/10.3390/galaxies5040073

**Chicago/Turabian Style**

Fromm, Christian M., Oliver Porth, Ziri Younsi, Yosuke Mizuno, Mariafelica De Laurentis, Hector Olivares, and Luciano Rezzolla.
2017. "Radiative Signatures of Parsec-Scale Magnetised Jets" *Galaxies* 5, no. 4: 73.
https://doi.org/10.3390/galaxies5040073