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QSO B0738+313

QSO B0738+313 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 QSO B0738+313 rather than just read about it. In short: QSO B0738+313 or B2 0738+313, is a quasar located in the constellation of Gemini. It has a redshift of (z) 0.630 and it was first discovered as an astronomical radio source in 1968 by astronomers who designated it as OI 363.

QSO B0738+313 — main illustration
QSO B0738+313 — illustration

Key takeaways

  • QSO B0738+313 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect QSO B0738+313 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of QSO B0738+313 from memory before moving on to harder problems.

Reference excerpt

QSO B0738+313 or B2 0738+313, is a quasar located in the constellation of Gemini. It has a redshift of (z) 0.630 and it was first discovered as an astronomical radio source in 1968 by astronomers who designated it as OI 363. The object has a radio spectrum appearing as flat making it a flat-spectrum radio quasar but also a gigahertz-peaked spectrum source.

Description QSO B0738+313 is classified as a core-dominated radio-loud quasar with an X-ray luminosity of L0.1-10 KeV ~ 45 erg s−1. However, the polarization level of the object is low. When observed by astronomers during R-band monitoring for four nights, its light curve was described as clear and almost sinusoidal with a few variations occurring on 21 January and 22 December 2006. In its spectrum, the quasar displays two dampened Lyman-alpha absorption-line systems located at redshifts of (z) 0.0912 and (z) 0.2212, making these the lowest known absorption-line systems of its kind. Two other faint companions were found, although not relating to the quasar. The quasar has a compact radio structure. When imaged with the Very Long Baseline Array at 15 GHz, it has two strong components. The first component is found weakly polarized at 0.5% with an inverted spectrum, while the other is polarized by around 1.5%. There are also weak and diffused radio lobes on each side of a much stronger radio component. Very Long Baseline Interferometry imaging at six centimeters showed the structure has an unresolved radio core, a small surface brightness radio emission surrounding the source and a jet located in north-south which extends by 5 milliarcseconds. This jet also displays a sharp bend at 45° towards the south-west direction with a knot at its bend.

X-ray jet An X-ray jet was discovered in QSO B0738+313 by Chandra X-ray observatory in March 2003. Based on results, the X-ray jet has an extent of 200 kiloparsecs and is narrow. Observations also showed the X-ray jet is curving as well, which then follows the path of a radio structure south of the quasar and terminating at a hotspot located within the southernmost part of a radio lobe. As it moves further from the core, the jet emission becomes fainter. Astronomers found the X-ray emission is centered strongly towards the jet's direction, 3.8 arcseconds south from the radio core suggesting location of innermost components of the jet.

References

External links QSO B0738+313 on SIMBAD

Illustrations

QSO B0738+313 illustration

Worked examples

Example 1 — a first encounter with QSO B0738+313

Start with the simplest possible case. Write down what QSO B0738+313 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 QSO B0738+313 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 QSO B0738+313 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 QSO B0738+313

In research
QSO B0738+313 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 QSO B0738+313 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
QSO B0738+313 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Active galaxies, Astronomical objects discovered in 1968, Gemini (constellation), so understanding it makes those chapters shorter.
In everyday life
Look for QSO B0738+313 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 QSO B0738+313 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what QSO B0738+313 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 QSO B0738+313 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is QSO B0738+313 in simple terms?

QSO B0738+313 or B2 0738+313, is a quasar located in the constellation of Gemini. It has a redshift of (z) 0.630 and it was first discovered as an astronomical radio source in 1968 by astronomers who designated it as OI 363.

Why does QSO B0738+313 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 QSO B0738+313?

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 QSO B0738+313.

Tags

  • Active galaxies
  • Astronomical objects discovered in 1968
  • Gemini (constellation)
  • Quasars
  • SDSS objects
  • Seyfert galaxies

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