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## VLBI Studies of Tanami Radio Galaxies

Труды ИПА РАН, вып. 41, 3–8 (2017)

Ключевые слова: VLBI, AGN, γ-rays, Radio galaxies

### Аннотация

Radio galaxies are relatively faint at γ-ray energies, where they make up only 1–2% of all AGN detected by Fermi-LAT. However, they offer a unique perspective to study the intrinsic properties of AGN jets. For this reason, the combination of γ-ray and multi-wavelength data with high-resolution VLBI monitoring is a powerful tool to tackle the basic unanswered questions about AGN jets. Here we present preliminary results from a sample study of radio galaxies in the Southern hemisphere observed by the TANAMI VLBI monitoring program. We obtain highresolution maps at 8.4 and 22.3 GHz, and study the jet kinematics using multi-epoch data. We present a preliminary kinematic analysis for the peculiar γ-ray AGN PKS 0521−36.

### Цитирование

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RIS
R. Angioni, F. Rösch, E. Ros, M. Kadler, R. Ojha, C. Müller, R. Schulz. VLBI Studies of Tanami Radio Galaxies // Труды ИПА РАН. — 2017. — Вып. 41. — С. 3–8. @article{angioni2017, abstract = {Radio galaxies are relatively faint at γ-ray energies, where they make up only 1–2% of all AGN detected by Fermi-LAT. However, they offer a unique perspective to study the intrinsic properties of AGN jets. For this reason, the combination of γ-ray and multi-wavelength data with high-resolution VLBI monitoring is a powerful tool to tackle the basic unanswered questions about AGN jets. Here we present preliminary results from a sample study of radio galaxies in the Southern hemisphere observed by the TANAMI VLBI monitoring program. We obtain highresolution maps at 8.4 and 22.3 GHz, and study the jet kinematics using multi-epoch data. We present a preliminary kinematic analysis for the peculiar γ-ray AGN PKS 0521−36.}, author = {R. Angioni and F. Rösch and E. Ros and M. Kadler and R. Ojha and C. Müller and R. Schulz}, issue = {41}, journal = {Труды ИПА РАН}, keyword = {VLBI, AGN, γ-rays, Radio galaxies}, pages = {3--8}, title = {VLBI Studies of Tanami Radio Galaxies}, url = {http://iaaras.ru/library/paper/1694/}, year = {2017} } TY - JOUR TI - VLBI Studies of Tanami Radio Galaxies AU - Angioni, R. AU - Rösch, F. AU - Ros, E. AU - Kadler, M. AU - Ojha, R. AU - Müller, C. AU - Schulz, R. PY - 2017 T2 - Труды ИПА РАН IS - 41 SP - 3 AB - Radio galaxies are relatively faint at γ-ray energies, where they make up only 1–2% of all AGN detected by Fermi-LAT. However, they offer a unique perspective to study the intrinsic properties of AGN jets. For this reason, the combination of γ-ray and multi-wavelength data with high-resolution VLBI monitoring is a powerful tool to tackle the basic unanswered questions about AGN jets. Here we present preliminary results from a sample study of radio galaxies in the Southern hemisphere observed by the TANAMI VLBI monitoring program. We obtain highresolution maps at 8.4 and 22.3 GHz, and study the jet kinematics using multi-epoch data. We present a preliminary kinematic analysis for the peculiar γ-ray AGN PKS 0521−36. UR - http://iaaras.ru/library/paper/1694/ ER -