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Immo Appenzeller

Immo Appenzeller 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 Immo Appenzeller rather than just read about it. In short: Immo Appenzeller (born May 13, 1940 in Urach, Württemberg) is a German astronomer. Career Source: Appenzeller studied physics at the University of Tübingen from 1959 on.

Immo Appenzeller — main illustration
Immo Appenzeller — illustration

Key takeaways

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

Reference excerpt

Immo Appenzeller (born May 13, 1940 in Urach, Württemberg) is a German astronomer.

Career Source: Appenzeller studied physics at the University of Tübingen from 1959 on. In 1961 he moved to Göttingen to study physics and astronomy at the University of Göttingen. He received his doctorate in 1966 with a thesis entitled Investigation of the structure of the galactic magnetic field in Cygnus and Orion using polarization measurements of starlight supervised by Alfred Behr. From 1964 to 1966 Appenzeller was research assistant at the Yerkes Observatory of the University of Chicago, and in 1967 he was appointed as an assistant at the Göttingen university observatory. After his habilitation in 1970 he became a private lecturer at the Göttinger university observatory. In 1972 he was a guest professor at the University of Tokyo, and in 1974 he was promoted to adjunct professor. In 1975 he was named director of the state observatory Heidelberg-Königstuhl state observatory and full professor of astronomy at the University of Heidelberg. In 1982/83 he was invited as guest scientist at the University of Arizona. In 1985/86 he served as Dean of the Faculty of Physics and Astronomy in Heidelberg. From 1998 to 2000 he was also acting director of the Max Planck Institute for Astronomy. He retired in 2005. Appenzeller supervised the doctoral theses of about twenty students, about a third of which continued working in astronomy.

Research Appenzeller conducted both observational and theoretical research and was also active in developing astronomical instruments. He was in particular project manager for the FORS instrument of the Very Large Telescope at ESO (European Southern Observatory) in Chile. He made significant contributions to several research fields, including star formation, stellar evolution, high redshift galaxies, active galaxies and quasars, massive luminous stars, and cosmic X-ray sources.

Honors Appenzeller is an "External Scientific Member" of the Max Planck Institute for Astronomy in Heidelberg. He is a member of the Heidelberg Academy of Sciences. From 1994 to 1997 he was Secretary General of the International Astronomical Union. In 2002 he received the Gay Lussac Humboldt Prize. In 1991, the asteroid (2373) Immo was named after him. In 2015 he was awarded the Karl Schwarzschild Medal for his outstanding contributions to astronomy.

Selected publications The first selection criterion for bibliographic references quoted in this section is the number of normalized citations, i.e., the total number of citations divided by the number of authors of the publication, as given by the Astrophysics Data System at the date of writing. Furthermore, only one reference is kept for each research subfield.

Appenzeller, I. and Mundt, R., “T Tauri stars”, Astronomy and Astrophysics Review, 1, 291–334, 1989 Appenzeller, I., “The evolution of a vibrationally unstable main-sequence star of 130 M sun.”, Astronomy & Astrophysics, 5, 355, 1970 Bouvier, J. and Appenzeller, I., “A magnitude-limited spectroscopic and photometric survey of rho Ophiuchus X-ray sources.”, Astronomy & Astrophysics Supplement Series, 92, 481–516, 1992 Appenzeller, I., “Polarimetric Observations of Nearby Stars in the Directions of the Galactic Poles and the Galactic Plane”, The Astrophysical Journal, 151, 907, 1968. doi:10.1086/149492 Zickgraf, F. J., Wolf, B., Stahl, O., Leitherer, C., and Appenzeller, I., “B(e)-supergiants of the Magellanic Clouds.”, Astronomy & Astrophysics, 163, 119–134, 1986

Books High redshift galaxies - light from the early universe, Springer 2009 Introduction to Astronomical Spectroscopy, Cambridge Verlag 2013

References

Illustrations

Immo Appenzeller illustration

Worked examples

Example 1 — a first encounter with Immo Appenzeller

Start with the simplest possible case. Write down what Immo Appenzeller 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 Immo Appenzeller 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 Immo Appenzeller 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 Immo Appenzeller

In research
Immo Appenzeller 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 Immo Appenzeller 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
Immo Appenzeller is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1940 births, Academic staff of Heidelberg University, German astronomers, so understanding it makes those chapters shorter.
In everyday life
Look for Immo Appenzeller 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 Immo Appenzeller in 20 minutes

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

Frequently asked questions

What is Immo Appenzeller in simple terms?

Immo Appenzeller (born May 13, 1940 in Urach, Württemberg) is a German astronomer. Career Source: Appenzeller studied physics at the University of Tübingen from 1959 on.

Why does Immo Appenzeller 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 Immo Appenzeller?

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 Immo Appenzeller.

Tags

  • 1940 births
  • Academic staff of Heidelberg University
  • German astronomers
  • Living people
  • Max Planck Institute directors
  • People from Bad Urach
  • University of Göttingen alumni
  • University of Tübingen alumni

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