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NRAO 140

NRAO 140 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 NRAO 140 rather than just read about it. In short: NRAO 140 is a quasar located in the constellation of Perseus, noted for its low frequency variability. It has a redshift of (z) 1.258, first discovered in 1973 by Duncan Agnew and Halton Arp as an astronomical radio source, whom they catalogued it as 4C 32.14.

NRAO 140 — main illustration
NRAO 140 — illustration

Key takeaways

  • NRAO 140 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect NRAO 140 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NRAO 140 from memory before moving on to harder problems.

Reference excerpt

NRAO 140 is a quasar located in the constellation of Perseus, noted for its low frequency variability. It has a redshift of (z) 1.258, first discovered in 1973 by Duncan Agnew and Halton Arp as an astronomical radio source, whom they catalogued it as 4C 32.14.

Description NRAO 140 is classified as a radio-selected blazar (RBL) based on European X-ray Observatory Satellite (EXOSAT) observations. However the object has no presence of either long-term or rapid fluxes. Its radio spectrum is flat, making it a flat-spectrum radio quasar, but also exhibiting radio and X-ray fluxes that lasted between 1979 and 1985. The brightness temperature of NRAO 140 is estimated to be between 5 × 1015 and 5 × 1014 Kelvin. A low frequency outburst was detected in NRAO 140 by the Very Long Baseline Array (VLBI) observations, peaking in 1981 with the component undergoing a decrease in brightness levels as the outburst faded. Between August 7 and 9 in 1986, the object displayed rising levels in K flux from 1.25 ± 0.06 mJy to around 1.54 ± 0.05 mJy in a span of two days during the observation campaign. Radio imaging made by Very Large Array (VLA) at both 21 and 6 centimeters (cm) shows the structure of NRAO 140 is made up of only a single secondary component with a position angle of 150°. Other radio images made by the Westerbork Synthesis Radio Telescope shows NRAO 140 has two components located on both sides of the radio core, consisting of a southwestern component at a position angle of 149° and a northeastern component at a position angle of -31° opposed to images made by VLA. VLBI observations also shows evidence of superluminal motion in several components separating at an angular rate of 0.10-0.14 milliarcseconds. The jet in NRAO 140 is found to bend slightly towards the south direction from the radio core with detections of polarized flux in its jet components. In additional, the position angle of the jet is found nearly perpendicular towards the jet's axis, with the jet itself having a faraday rotation measure gradient extended by 8 milliarcseconds from the core. By constraining the upper limits of the jet's viewing angle, the jet is confirmed to have a linear extent greater than 350 parsecs.

References

External links NRAO 140 by SIMBAD NRAO 140 by NASA/IPAC Database

Illustrations

NRAO 140 illustration

Worked examples

Example 1 — a first encounter with NRAO 140

Start with the simplest possible case. Write down what NRAO 140 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 NRAO 140 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 NRAO 140 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 NRAO 140

In research
NRAO 140 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 NRAO 140 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
NRAO 140 is common in secondary-school and first-year university syllabi. It links to neighbouring topics 4C objects, Active galaxies, Astronomical objects discovered in 1973, so understanding it makes those chapters shorter.
In everyday life
Look for NRAO 140 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 NRAO 140 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NRAO 140 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 NRAO 140 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NRAO 140 in simple terms?

NRAO 140 is a quasar located in the constellation of Perseus, noted for its low frequency variability. It has a redshift of (z) 1.258, first discovered in 1973 by Duncan Agnew and Halton Arp as an astronomical radio source, whom they catalogued it as 4C 32.14.

Why does NRAO 140 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 NRAO 140?

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 NRAO 140.

Tags

  • 4C objects
  • Active galaxies
  • Astronomical objects discovered in 1973
  • Blazars
  • LEDA objects
  • Perseus (constellation)
  • Quasars

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