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Chapter 16 Quasars and Active Galaxies

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Chapter 16. Quasars and Active Galaxies. What do you think?. What do quasars look like? What powers a quasar?. Galaxy Cygnus A. This galaxy has a red shift corresponding to 6% the speed of light or 750 million light-years away. Quasars look like stars but have huge redshifts. - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: Chapter 16

Chapter 16

Quasars and Active Galaxies

Page 2: Chapter 16

What do you think?

• What do quasars look like?

• What powers a quasar?

Page 3: Chapter 16

Galaxy Cygnus A

This galaxy has a red shift corresponding to 6% the speed of light or 750 million light-years away

Page 4: Chapter 16

Quasars look like stars but have huge redshifts

• object with a spectrum much like a dim star

• highly red shifted

• enormous recessional velocity

• huge distance (ala Hubble’s Law)

• must be enormously bright to be visible at such a great distance

• Quasi-stellar object

• QSO or Quasar

Page 5: Chapter 16

This object that looks like a star must be

enormously luminous - its redshift indicates it is 4 billion light years

away!!

Page 6: Chapter 16

3C 273’s spectral lines are greatly redshifted

This change implies a distance of 2 billion light years

Page 7: Chapter 16

A quasar emits a huge amount of energy from a small volume

Such rapid changes in brightness can only result from changes small objects

Page 8: Chapter 16

Active Galaxies bridge the energy gap between ordinary

galaxies and quasars• peculiar galaxies (pec)

– appear to be blowing themselves apart

Page 9: Chapter 16
Page 10: Chapter 16

Active Galaxies bridge the energy gap between ordinary

galaxies and quasars• peculiar galaxies (pec)

– appear to be blowing themselves apart

• Seyfert galaxies– luminous, star-like nuclei with strong emission

lines

Page 11: Chapter 16
Page 12: Chapter 16

Active Galaxies bridge the energy gap between ordinary

galaxies and quasars• peculiar galaxies (pec)

– appear to be blowing themselves apart

• Seyfert galaxies– luminous, star-like nuclei with strong emission

lines

• BL Lacertae objects (BL Lacs)– featureless spectrum with a brightness that can

vary by a factor of 15 times in a few months.

Page 13: Chapter 16
Page 14: Chapter 16

Radio image of Cygnus A showing a small but very bright radio galaxy in the middle of the 320,000 ly wide lobes

Page 15: Chapter 16

Active galaxies lie at the center of double radio sources

Page 16: Chapter 16

Supermassive black holes lurk at the centers of some galaxies

• High resolution spectroscopy allows astronomers to peak at the motion of gas near centers of galaxies

• Some galaxies exhibit high-velocity jets of material leaving the center

• Observations suggest that the centers of some galaxies are incredibly massive

• All of this suggests the existence of supermassive black holes

Page 17: Chapter 16

Galaxy (which is actually

quite large)

Intergalactic gas jet

Giant Gas Clouds

(surrounding the galaxy)

Page 18: Chapter 16

Jets of matter ejected from around a black hole

may explain quasars and active galaxies

Page 19: Chapter 16

Jets of matter ejected from around a black hole may explain quasars and active galaxies

Page 20: Chapter 16

From where you observe it might make all the difference ...

Page 21: Chapter 16

What did you think?

• What do quasars look like?They look like stars but spew out immense

energy

• What powers a quasar?A quasar is a galaxy powered by a supermassive

black hole at its center.

Page 22: Chapter 16

Self-Check

1: Describe the observable properties of quasars and indicate how they are identified.

2: Explain why intrinsic properties of quasars are so difficult to explain.

3: List the various types of active galaxies and discuss how each might be related to quasars.

4: Discuss the observations that seem to be consistent with the presence of supermassive black holes in most galaxies.