Hypernova and gamma-ray burst remnants as tev unidentified sources

Kunihito Ioka, Peter Istvan Meszaros

Research output: Contribution to journalArticle

16 Citations (Scopus)

Abstract

We investigate hypernova (hyper-energetic supernova) and gamma-ray burst (GRB) remnants in our Galaxy as TeV gamma-ray sources, particularly in the role of potential TeV unidentified sources, which have no clear counterpart at other wavelengths. We show that the observed bright sources in the TeV sky could be dominated by GRB/hypernova remnants, even though they are fewer than supernova remnants (SNRs). If this is the case, TeV SNRs are more extended (and more numerous) than deduced from current observations. In keeping with their role as cosmic ray accelerators, we discuss hadronic gamma-ray emission from πo decay, from β decay followed by inverse Compton emission, and propose a third novel process of TeV gamma-ray emission arising from the decay of accelerated radioactive isotopes such as 56Co entrained by relativistic or semi-relativistic jets in GRBs/hypernovae. We discuss the relevant observational signatures which could discriminate between these three mechanisms.

Original languageEnglish (US)
Pages (from-to)1337-1342
Number of pages6
JournalAstrophysical Journal
Volume709
Issue number2
DOIs
StatePublished - Feb 1 2010

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supernova remnants
gamma ray bursts
decay
energetics
gamma rays
radioactive isotopes
cosmic ray
supernovae
sky
cosmic rays
accelerators
signatures
isotope
galaxies
wavelength
wavelengths

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Ioka, Kunihito ; Meszaros, Peter Istvan. / Hypernova and gamma-ray burst remnants as tev unidentified sources. In: Astrophysical Journal. 2010 ; Vol. 709, No. 2. pp. 1337-1342.
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Hypernova and gamma-ray burst remnants as tev unidentified sources. / Ioka, Kunihito; Meszaros, Peter Istvan.

In: Astrophysical Journal, Vol. 709, No. 2, 01.02.2010, p. 1337-1342.

Research output: Contribution to journalArticle

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