4.3 Article

The gamma-ray Doppler factor determinations for a Fermi blazar sample

Journal

RESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume 13, Issue 3, Pages 259-269

Publisher

NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
DOI: 10.1088/1674-4527/13/3/002

Keywords

galaxies: active; galaxies: BL Lacertae objects; galaxies: quasars; galaxies: jets

Funding

  1. National Natural Science Foundation of China [11173009]
  2. National Basic Research Program of China (973 program) [2007CB815405]
  3. Bureau of Education of Guangzhou Municipality [11 Sui-Jiao-Ke[2009]]
  4. Guangdong Province Universities and Colleges Pearl River Scholar Funded Scheme (GDUPS)
  5. Yangcheng Scholar Funded Scheme [10A027S]
  6. Joint Laboratory for Optical Astronomy of Chinese Academy of Sciences

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Observations suggest that gamma-ray loud blazars are strongly beamed. The Fermi mission has detected many of blazars, which provide us with a good opportunity to investigate the emission mechanism and the beaming effect in the gamma-ray region. We compiled the X-ray observations for 138 Fermi blazars (54 flat spectrum radio quasars, 36 low-peaked BL Lacertae objects, and 48 high-peaked BL Lacertae objects) and calculated their Doppler factors, delta(gamma) . It is interesting that the calculated Doppler factors, delta(gamma), are strongly correlated with the gamma-ray luminosity.

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