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astronomy

PKS 0634−20

PKS 0634−20 is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand PKS 0634−20 rather than just read about it. In short: PKS 0634−20 is a powerful Fanaroff-Riley class Type II radio galaxy located in the constellation of Canis Major. It has a redshift of (z) 0.056 and was first discovered by astronomers who were conducting the Parkes catalogue survey at Parkes Observatory in 1964.

PKS 0634−20 — main illustration
PKS 0634−20 — illustration

Key takeaways

  • PKS 0634−20 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect PKS 0634−20 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of PKS 0634−20 from memory before moving on to harder problems.

Reference excerpt

PKS 0634−20 is a powerful Fanaroff-Riley class Type II radio galaxy located in the constellation of Canis Major. It has a redshift of (z) 0.056 and was first discovered by astronomers who were conducting the Parkes catalogue survey at Parkes Observatory in 1964. This object is also classified as a Type 2 Seyfert galaxy.

Description PKS 0634−20 is classified as a giant radio galaxy with a complex radio structure. When imaged with a 21 centimeter radio map, the structure is best described as a double-triple made up of seven components with an unresolved southern bright component. Observations made by the Westerbork Synthesis Radio Telescope found the outer edges of two components have a separation gap of 14 arcseconds. In addition, the components are narrow and configured, similar to 3C 236. Observations made with the Effelsberg 100-m Radio Telescope and Very Large Array, discovered there is a long radio emission bridge in PKS 0634−20. When imaged, the bridge is found extending to the outer collinear hotspots with its polarization degree varying from 8% to 30%. When travelling a far distance in terms of projection, there is a change in which the bridge becomes narrower and the polarization degree increases. Results also showed the hotspots located at north and south directions have polarization percentages of 5% and 20%. As mapping at 4".5 resolution also showed the same thing, this suggests either beam cancellation of the northern sub-parts of the hotspot or differential Faraday rotation. Imaging at high resolutions by the Australia Telescope Compact Array also showed the south hotspot has a significant sub-structure. The host of PKS 0634−20 is a normal elliptical galaxy lying in the poor cluster environment. According to imaging by the Anglo-Australian Telescope, the appearance of the galaxy is described as peculiar with a sign of a filamentary structure showing an extension into a northwest quadrant. There is an emission line nebula extending by 20 kiloparsecs from its central nucleus with molecular gas estimated to be 3 × 109 M☉. As its mass is greater than the warm gas in the galaxy, this indicates the nebula is radiation-bound. The large quantity of gas is believed to be acquired from either a spiral or a gas-rich galaxy. Strong doubly ionized oxygen narrow emission lines has been identified in the spectra of PKS 0634−20 with an extent of 70 kiloparsecs along its radio axis. Astronomers also suggested the galaxy might have a hidden quasar based on the discovery of a reddened source coinciding with its nucleus.

References

External links PKS 0634−20 on SIMBAD PKS 0634−20 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

PKS 0634−20 illustration

Worked examples

Example 1 — a first encounter with PKS 0634−20

Start with the simplest possible case. Write down what PKS 0634−20 claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to PKS 0634−20 before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about PKS 0634−20 ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of PKS 0634−20

In research
PKS 0634−20 appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses PKS 0634−20 in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
PKS 0634−20 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Active galaxies, Astronomical objects discovered in 1964, Canis Major, so understanding it makes those chapters shorter.
In everyday life
Look for PKS 0634−20 outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study PKS 0634−20 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what PKS 0634−20 means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain PKS 0634−20 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is PKS 0634−20 in simple terms?

PKS 0634−20 is a powerful Fanaroff-Riley class Type II radio galaxy located in the constellation of Canis Major. It has a redshift of (z) 0.056 and was first discovered by astronomers who were conducting the Parkes catalogue survey at Parkes Observatory in 1964.

Why does PKS 0634−20 matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study PKS 0634−20?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on PKS 0634−20.

Tags

  • Active galaxies
  • Astronomical objects discovered in 1964
  • Canis Major
  • Elliptical galaxies
  • IRAS catalogue objects
  • Principal Galaxies Catalogue objects
  • Radio galaxies
  • Seyfert galaxies

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