Busca avançada
Ano de início
Entree
(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

The relativistic parsec-scale jets of the blazars TXS 0506+056 and PKS 0502+049 and their possible association with gamma-ray flares and neutrino production

Texto completo
Autor(es):
Sumida, Viktor Y. D. [1, 2] ; Schutzer, A. de A. [3] ; Caproni, A. [1] ; Abraham, Z. [4]
Número total de Autores: 4
Afiliação do(s) autor(es):
[1] Univ Cidade Sao Paulo, Nucleo Astrofis, R Galvao Bueno 868, BR-01506000 Sao Paulo, SP - Brazil
[2] Univ Cruzeiro Sul, R Galvao Bueno 868, BR-01506000 Sao Paulo, SP - Brazil
[3] Univ Grenoble Alpes, IPAG, CNRS, F-38000 Grenoble - France
[4] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, R Matao 1226, Cidade Univ, BR-05508900 Sao Paulo, SP - Brazil
Número total de Afiliações: 4
Tipo de documento: Artigo Científico
Fonte: Monthly Notices of the Royal Astronomical Society; v. 509, n. 2, p. 1646-1663, JAN 2022.
Citações Web of Science: 0
Resumo

The physical nature of the mechanism responsible for the emission of neutrinos in active galactic nuclei (AGNs) has been matter of debate in the literature, with relativistic jets of radio-loud AGNs as possible candidates to be the sources of high-energy neutrinos. The most prominent candidate so far is the blazar TXS 0506+056, which is found to be associated with the neutrino event IceCube-170922A. Furthermore, the IceCube reported an excess of neutrinos towards TXS 0506+056 between September 2014 and March 2015, even though this association needs additional investigation, considering the presence of a nearby gamma-ray source, the quasar PKS 0502+049. Motivated by this, we studied the parsec-scale structures of TXS 0506+056 and PKS 0502+049 through radio interferometry at 8 and 15 GHz. We identified twelve jet components in TXS 0506+056 and seven components in PKS 0502+049. The most reliable jet components show superluminal speeds ranging from 9.5c to 66c in the case of TXS 0506+056, and from 14.3c to 59c for PKS 0502+049, which were used to estimate a lower (upper) limit for the Lorentz factor (jet viewing angle) for both sources. A novel approach using simultaneously the brightness temperature of the core region and the apparent speeds of the jet components allowed us to infer basic jet parameters for TXS 0506+056 at distinct epochs. We also found that the emergence of new jet components coincides with the occurrence of gamma-ray flares. Interestingly, two of these coincidences in the case of PKS 0502+049 and one for TXS 0506+056 seems to be correlated with neutrino events detected by the IceCube Observatory. (AU)

Processo FAPESP: 17/25651-5 - Estudos numéricos de objetos extragalácticos no universo local e em altos redshifts
Beneficiário:Anderson Caproni
Linha de fomento: Auxílio à Pesquisa - Regular
Processo FAPESP: 14/11156-4 - O que determina o crescimento da massa estelar de galáxias elípticas? Intrínseco ou ambiente: a saga contínua
Beneficiário:Reinaldo Ramos de Carvalho
Linha de fomento: Auxílio à Pesquisa - Temático