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Contribution from Star-forming Galaxies to the Cosmic Gamma-ray Background Radiation

  • Authors: Ryu Makiya, Tomonori Totani, and Masakazu A. R. Kobayashi

Makiya, Totani, & Kobayashi 2011 The Astrophysical Journal 728 158.

  • Provider: AAS Journals

Caption: Figure 1.

Top: correlation between the gamma-ray luminosity L γ (0.1–5 GeV) and the product of SFR and gas mass, ψ M gas. The solid line represents the best fit power-law L γ ∝ (ψ M gas) α with α taken as a free parameter. The dashed line represents a linear function fit with a fixed value of α = 1. Bottom: the same as the top panel, but for the correlation between L γ and SFR.

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