ǂa ǂpotential PeVatron candidate for the CTA in the northern hemisphere
Gaia Verna (Avtor), Saptashwa Bhattacharyya (Avtor), B. Marčun (Avtor), Judit Pérez Romero (Avtor), Samo Stanič (Avtor), Veronika Vodeb (Avtor), Serguei Vorobiov (Avtor), Gabrijela Zaharijas (Avtor), Marko Zavrtanik (Avtor), Danilo Zavrtanik (Avtor), Miha Živec (Avtor)

Povzetek

Recent observations of the gamma-ray source HAWC J2227+610 by Tibet AS+MD and LHAASO confirm the special interest of this source as a galactic PeVatron candidate in the northern hemi-sphere. HAWC J2227+610 emits Very High Energy (VHE) gamma-rays up to 500 TeV, from a region coincident with molecular clouds and significantly displaced from the nearby pulsar J2229+6114. Even if this morphology favours an hadronic origin, both leptonic or hadronic models can describe the current VHE gamma-ray emission. The morphology of the source is not well constrained by the present measurements and a better characterisation would greatly help the understanding of the underlying particle acceleration mechanisms. The Cherenkov Telescope Array (CTA) will be the future most sensitive Imaging Atmospheric Cherenkov Telescope and, thanks to its unprecedented angular resolution, could contribute to better constrain the nature of this source. The present work investigates the potentiality of CTA to study the morphology and the spectrum of HAWC J2227+610. For this aim, the source is simulated assuming the hadronic model proposed by the Tibet AS+MD collaboration, recently fitted on multi-wavelength data, and two spatial templates associated to the source nearby molecular clouds. Di˙erent CTA layouts and observation times are considered. A 3D map based analysis shows that CTA is able to significantly detect the extension of the source and to attribute higher detection significance to the simulated molecular cloud template compared to the alternative one. CTA data does not allow to disentangle the hadronic and the leptonic emission models. However, it permits to correctly reproduce the simulated parent proton spectrum characterized by a ∼ 500 TeV cuto˙.

Ključne besede

very-high energy gamma-rays;Cherenkov Telescope Array;

Podatki

Jezik: Angleški jezik
Leto izida:
Tipologija: 1.06 - Objavljeni znanstveni prispevek na konferenci (vabljeno predavanje)
Organizacija: UNG - Univerza v Novi Gorici
UDK: 539.1
COBISS: 164927747 Povezava se bo odprla v novem oknu
ISSN: 1824-8039
Št. ogledov: 90
Št. prenosov: 0
Ocena: 0 (0 glasov)
Metapodatki: JSON JSON-RDF JSON-LD TURTLE N-TRIPLES XML RDFA MICRODATA DC-XML DC-RDF RDF

Ostali podatki

Vrsta dela (COBISS): Delo ni kategorizirano
Strani: str. 1-11
Čas izdaje: 2022
ID: 19949760
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, ǂa ǂpotential PeVatron candidate for the CTA in the northern hemisphere
, ǂthe ǂworld’s largest VHE gamma-ray observatory
, layout, design and performance