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Cosmic Gamma-Ray Sources (2004)

Cosmic Gamma-Ray Sources

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"Cosmic Gamma-Ray Sources" by Ka Lok Cheng, Gustavo E. Romero is a astronomy book and space science reference focused on Equipment & Methods. Best for students, researchers, and serious astronomy enthusiasts.

Gamma-ray astronomy has undergone an enormous progress in the last 15 years. The success of satellite experiments like NASA's Comp ton Gamma-Ray Observatory and ESA's INTEGRAL mission, as well as of ground-based instruments have open new views into the high-energy Universe. Different classes of cosmic gamma-ray sources have been now detected at different energies, in addition to young radio pulsars and gamma-ray bursts, the classical ones. The new sources include radio quiet pulsars, microquasars, supernova remnants, starburst galaxies, ra dio galaxies, flat-spectrum radio quasars, and BL Lacertae objects. A large number of unidentified sources strongly suggests that this brief enumeration is far from complete. Gamma-ray bursts are now estab lished as extragalactic sources with tremendous energy output. There is accumulating evidence supporting the idea that massive stars and star forming regions can accelerate charged particles up to relativistic ener gies making them gamma-ray sources. Gamma-ray astronomy has also proved to be a powerful tool for cosmology imposing constraints to the background photon fields that can absorb the gamma-ray flux from dis tant sources. All this has profound implications for our current ideas about how particles are accelerated and transported in both the local and distant U niverse. The evolution of our knowledge on the gamma-ray sky has been so fast that is not easy for the non-specialist scientist and the graduate student to be aware of the full potential of this field or to grasp the fundamentals of a given topic in order to attempt some original contribution.

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Best For: Students and researchers interested in high-energy astrophysics and gamma-ray astronomy.
Focus: The detection and study of various cosmic gamma-ray sources using satellite and ground-based instruments.
Covers: Progress in gamma-ray astronomy over the last 15 years, including observations from NASA's Compton Gamma-Ray Observatory and ESA's INTEGRAL mission.
Why It Matters: Understanding gamma-ray sources provides insights into energetic processes in the universe beyond classical sources like pulsars and gamma-ray bursts.

"Cosmic Gamma-Ray Sources" by Ka Lok Cheng, Gustavo E. Romero is a astronomy book and space science reference focused on Equipment & Methods. Best for students, researchers, and serious astronomy enthusiasts.

Topic: Equipment & Methods

Author: Ka Lok Cheng, Gustavo E. Romero

Who this is for:

  • Astronomy students
  • Researchers and advanced hobbyists
  • Readers exploring space science topics

Why this book matters: It matters because it helps readers build a stronger understanding of astronomy concepts, observations, and scientific ideas related to space.

Gamma-ray astronomy has undergone an enormous progress in the last 15 years. The success of satellite experiments like NASA's Comp ton Gamma-Ray Observatory and ESA's INTEGRAL mission, as well as of ground-based instruments have open new views into the high-energy Universe. Different classes of cosmic gamma-ray sources have been now detected at different energies, in addition to young radio pulsars and gamma-ray bursts, the classical ones. The new sources include radio quiet pulsars, microquasars, supernova remnants, starburst galaxies, ra dio galaxies, flat-spectrum radio quasars, and BL Lacertae objects. A large number of unidentified sources strongly suggests that this brief enumeration is far from complete. Gamma-ray bursts are now estab lished as extragalactic sources with tremendous energy output. There is accumulating evidence supporting the idea that massive stars and star forming regions can accelerate charged particles up to relativistic ener gies making them gamma-ray sources. Gamma-ray astronomy has also proved to be a powerful tool for cosmology imposing constraints to the background photon fields that can absorb the gamma-ray flux from dis tant sources. All this has profound implications for our current ideas about how particles are accelerated and transported in both the local and distant U niverse. The evolution of our knowledge on the gamma-ray sky has been so fast that is not easy for the non-specialist scientist and the graduate student to be aware of the full potential of this field or to grasp the fundamentals of a given topic in order to attempt some original contribution.

AuthorKa Lok Cheng, Gustavo E. Romero
PublisherSpringer Science & Business Media
Published2004-10-25
ISBN-139781402022555
BindingHardcover
Pages428
LanguageEnglish
SubjectsScience
TopicEquipment & Methods
SeriesAstrophysics and Space Science Library

Format: Hardcover

Length: 428 pages

Language: English

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