Broad-line region

Definition

The broad-line region refers to a zone surrounding a supermassive black hole in an active galactic nucleus, where gas and dust are moving at high velocities, resulting in the broadening of emission lines observed in the spectrum of quasars. This region is crucial in understanding the dynamics and physics of material being accreted by the black hole and the characteristics of the surrounding environment.

5 Must Know Facts For Your Next Test

1. The broad-line region typically extends from about 10 to 100 light-days from the supermassive black hole, where the high velocity of gas clouds results in Doppler broadening of spectral lines.
2. Observations of broad emission lines can provide insights into the mass of the black hole, as well as the dynamics and temperature of the gas in this region.
3. The broad-line region is composed of various ionized elements, including hydrogen, helium, and heavier elements, which contribute to the unique spectral signatures observed in quasars.
4. Variability in the emission lines over time can indicate changes in the physical conditions within the broad-line region, which may correlate with fluctuations in accretion rates onto the black hole.
5. Research on the broad-line region has significant implications for our understanding of galaxy formation and evolution, as these regions play a key role in how energy is released into the surrounding environment.

Review Questions

• How does the movement of gas in the broad-line region affect the spectral lines observed from quasars?
  • The movement of gas in the broad-line region affects spectral lines through a phenomenon known as Doppler broadening. As gas clouds orbit at high velocities around the supermassive black hole, their emitted light is shifted depending on their motion relative to the observer. This results in wider emission lines compared to those seen in stationary sources, providing crucial information about the dynamics and conditions present within this region.
• Discuss the significance of studying broad emission lines for understanding supermassive black holes and their environments.
  • Studying broad emission lines is significant because they offer insights into the properties of supermassive black holes and their immediate environments. The characteristics of these lines can reveal information about the mass and spin of the black hole, as well as the kinematics and composition of the surrounding gas. Furthermore, understanding these features contributes to our knowledge of how quasars impact galaxy evolution and interact with their host galaxies.
• Evaluate how variations in emission lines from the broad-line region can inform astronomers about changes in accretion processes onto supermassive black holes.
  • Variations in emission lines from the broad-line region can provide critical data on changes occurring during accretion processes. When there are shifts or changes in intensity within these lines, it may indicate fluctuations in gas density or temperature related to changing accretion rates onto the black hole. By monitoring these variations over time, astronomers can better understand the dynamics at play within active galactic nuclei and how they influence galaxy growth and activity.

Related terms

Quasar:

A quasar is an extremely luminous active galactic nucleus powered by a supermassive black hole, emitting vast amounts of energy across the electromagnetic spectrum.

Emission Lines: Emission lines are specific wavelengths of light emitted by atoms in a gas when they transition from a higher energy state to a lower one, often seen in the spectra of celestial objects.

Accretion Disk: An accretion disk is a structure formed by diffused material in orbital motion around a central body, such as a black hole, where friction and gravitational forces heat the material and generate radiation.