Contribution from normal and starburst galaxies to the extragalactic gamma-ray background (EGRB)

Debbijoy Bhattacharya, Parameswaran Sreekumar

Research output: Contribution to journalArticle

7 Citations (Scopus)

Abstract

The extragalactic diffuse emission at γ-ray energies has interesting cosmological implications since these photons suffer little or no attenuation during their propagation from the site of origin. The emission could originate from either truly diffuse processes or from unresolved point sources such as AGNs, normal galaxies and starburst galaxies. Here, we examine the unresolved point source origin of the extragalactic γ-ray background emission from normal galaxies and starburst galaxies. γ-ray emission from normal galaxies is primarily coming from cosmic-ray interactions with interstellar matter and radiation (∼90%) along with a small contribution from discrete point sources (∼10%). Starburst galaxies are expected to have enhanced supernovae activity which leads to higher cosmic-ray densities, making starburst galaxies sufficiently luminous at γ-ray energies to be detected by the current γ-ray mission (Fermi Gamma-ray Space Telescope).

Original languageEnglish
Pages (from-to)509-519
Number of pages11
JournalResearch in Astronomy and Astrophysics
Volume9
Issue number5
DOIs
Publication statusPublished - 2009

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starburst galaxies
rays
gamma rays
galaxies
point source
point sources
cosmic ray
cosmic rays
interstellar radiation
interstellar matter
Fermi Gamma-ray Space Telescope
energy
supernovae
attenuation
propagation
photons
interactions

All Science Journal Classification (ASJC) codes

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

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abstract = "The extragalactic diffuse emission at γ-ray energies has interesting cosmological implications since these photons suffer little or no attenuation during their propagation from the site of origin. The emission could originate from either truly diffuse processes or from unresolved point sources such as AGNs, normal galaxies and starburst galaxies. Here, we examine the unresolved point source origin of the extragalactic γ-ray background emission from normal galaxies and starburst galaxies. γ-ray emission from normal galaxies is primarily coming from cosmic-ray interactions with interstellar matter and radiation (∼90{\%}) along with a small contribution from discrete point sources (∼10{\%}). Starburst galaxies are expected to have enhanced supernovae activity which leads to higher cosmic-ray densities, making starburst galaxies sufficiently luminous at γ-ray energies to be detected by the current γ-ray mission (Fermi Gamma-ray Space Telescope).",
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Contribution from normal and starburst galaxies to the extragalactic gamma-ray background (EGRB). / Bhattacharya, Debbijoy; Sreekumar, Parameswaran.

In: Research in Astronomy and Astrophysics, Vol. 9, No. 5, 2009, p. 509-519.

Research output: Contribution to journalArticle

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