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28 May 2023 to 2 June 2023
Tianfu Cosmic Ray Research Centre
Asia/Shanghai timezone

Exploring the Emission Mechanisms of Mrk 180 with long term X-ray and Gamma-ray data

Not scheduled
10m
Tianfu Cosmic Ray Research Centre

Tianfu Cosmic Ray Research Centre

No. 1500 Kezhi Road, Tianfu New Area, Chengdu, Chin
poster

Speaker

Dr Sandeep Kumar MONDAL (Raman Research Institute)

Description

Markarian (Mrk) 180 is a BL Lacertae (BL Lac) object located at a redshift of 0.045 and a potential candidate for high-energy cosmic ray acceleration.
We have analyzed the Fermi-LAT gamma-ray data of Mrk 180 collected over a period of 12.8 years. We have also analyzed Swift X-ray, ultraviolet & optical, and XMM-Newton X-ray data to construct the multi-wavelength SED. The SED has been modelled with one-zone pure leptonic and lepto-hadronic scenarios to explain the underlying physics of multi-wavelength emission. We have done a comparative study between these pure leptonic and lepto-hadronic models. Moreover, an earlier study has associated Mrk 180 with the Telescope Array (TA) hotspot of UHECRs at E>57 EeV motivates us to check whether ultrahigh energy protons
and iron nuclei can reach the earth from Mrk 180. In this poster, I shall give an overview of our work on this source.

Presentation materials

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