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The Electromagnetic Spectrum02:37

The Electromagnetic Spectrum

The electromagnetic spectrum consists of all the types of electromagnetic radiation arranged according to their frequency and wavelength. Each of the various colors of visible light has specific frequencies and wavelengths associated with them, and you can see that visible light makes up only a small portion of the electromagnetic spectrum. Because the technologies developed to work in various parts of the electromagnetic spectrum are different, for reasons of convenience and historical...
The Electromagnetic Spectrum01:24

The Electromagnetic Spectrum

Electromagnetic waves are categorized according to their wavelengths and frequencies, giving the electromagnetic spectrum. These waves are classified as radio, infrared, ultraviolet, etc. Radio waves refer to electromagnetic radiation with wavelengths ranging from millimeters to kilometers. Radio waves are commonly used for audio communications (i.e., radios) and typically result from an alternating current in the wires of a broadcast antenna. They cover a broad wavelength range and are used...
Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Types of Radioactivity03:23

Types of Radioactivity

The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Emission Spectra02:39

Emission Spectra

When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...

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Video Experimental Relacionado

Updated: Jul 11, 2026

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
09:38

Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

Published on: December 18, 2015

Los cuásares, los blazars y los rayos gamma.

C D Dermer, R Schlickeiser

    Science (New York, N.Y.)
    |September 18, 1992
    PubMed
    Resumen

    El Compton Gamma Ray Observatory (CGRO) descubrió 13 nuevas fuentes extragalácticas de rayos gamma, en su mayoría blazars, ampliando nuestra comprensión de los núcleos galácticos activos. Estos hallazgos revelan procesos energéticos en el universo, originados en agujeros negros supermasivos.

    Área de la Ciencia:

    • Astrofísica de altas energías de alta energía.
    • La astronomía extragaláctica es la astronomía extragaláctica.
    • Física de los rayos cósmicos Física de los rayos cósmicos

    Sus antecedentes:

    • Anteriormente, sólo el cuásar 3C 273 era conocido como una fuente extragaláctica de radiación gamma de >100 MeV.
    • El Energetic Gamma Ray Experiment Telescope (EGRET) en el Compton Gamma Ray Observatory (CGRO) fue lanzado para estudiar el cielo de rayos gamma.

    Objetivo del estudio:

    • Identificar y caracterizar fuentes extragalácticas de radiación gamma de alta energía.
    • Investigar las propiedades de estas fuentes y su relación con los núcleos galácticos activos (AGN).

    Principales métodos:

    • Utilizando los datos del Telescopio Experimental de Rayos Gamma Energéticos (EGRET) a bordo del Observatorio de Rayos Gamma de Compton (CGRO).

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  • Analizando las emisiones de rayos gamma de fuentes extragalácticas.
  • Correlación de los hallazgos de rayos gamma con observaciones de múltiples longitudes de onda (radio, óptica) para identificar las propiedades del blazar.
  • Principales resultados:

    • El descubrimiento de 13 nuevas fuentes de rayos gamma extragalácticas en menos de un año de observaciones de CGRO, elevando el total a 14.
    • Todas las fuentes identificadas exhiben características de blazar, incluyendo alta polarización óptica, variabilidad y emisión de radio de espectro plano.
    • Es probable que estas fuentes sean raras, galaxias de radio alineadas favorablemente y cuásares con chorros relativistas.

    Conclusiones:

    • El instrumento EGRET del CGRO ha aumentado significativamente el número de fuentes extragalácticas conocidas de rayos gamma.
    • Los blazars son fuentes dominantes de rayos gamma de alta energía más allá de nuestra galaxia.
    • Las observaciones de rayos gamma proporcionan información crucial sobre los motores centrales de las AGN y los procesos astrofísicos extremos.