Aachen 2019 – wissenschaftliches Programm

Bereiche | Tage | Auswahl | Suche | Aktualisierungen | Downloads | Hilfe

T: Fachverband Teilchenphysik

T 39: Gamma-Astronomie I

T 39.5: Vortrag

Dienstag, 26. März 2019, 17:10–17:25, S14

Multiwavelength Analysis of NGC 1275/3C 84 using MAGIC, FermiLAT and VLBA Data — •Lena Linhoff and Kevin Schmidt — TU Dortmund

The radio galaxy 3C 84 is a well studied source of radio emission and was detected as misaligned blazar NGC 1275 also in the very high energy regime by gamma ray detectors like MAGIC and FermiLAT. Radio images show multiple and variable emission regions within the core of the galaxy moving away from the innermost core component. In the gamma ray regime the source is known to be variable in flux and experienced some flaring activity in 2017. The Radio flux shows a slight but constant increase in radio emission until mid 2016. Since the origin of the gamma ray emission is still unclear, multiwavelength studies are performed to explain the behavoir of the source. This talk presents a multiwavelength analysis using data taken by MAGIC and the VLBA from 2005 until 2018.