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Gloria Suzanne Koenigsberger Horowitz

Gloria Suzanne Koenigsberger Horowitz 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 Gloria Suzanne Koenigsberger Horowitz rather than just read about it. In short: Gloria Suzanne Koenigsberger Horowitz is a Mexican astrophysicist and professor working at the National Autonomous University of Mexico (UNAM). Her areas of expertise are in stellar spectroscopy, massive stars and binary interaction effects.

Gloria Suzanne Koenigsberger Horowitz — main illustration
Gloria Suzanne Koenigsberger Horowitz — illustration

Key takeaways

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

Reference excerpt

Gloria Suzanne Koenigsberger Horowitz is a Mexican astrophysicist and professor working at the National Autonomous University of Mexico (UNAM). Her areas of expertise are in stellar spectroscopy, massive stars and binary interaction effects. She was director of UNAM's Instituto de Astronomía (1990-1998) and a leading member of the team that succeeded in establishing the first connection to the Internet in Mexico in 1989.

Academic career Gloria Koenigsberger was born in Mexico City. She obtained a licentiate in Physics at the UNAM School of Sciences, graduating in 1978, and a doctorate in Astronomy at Pennsylvania State University in 1983, under the direction of Lawrence H. Auer. She served as Director of the Instituto de Astronomía of UNAM from December 4, 1990, until early December 1998, during which time the Institute initiated collaborative programs with several US observatories aimed at improving the San Pedro Mártir (SPM) National Observatory infrastructure and promoting the construction of a large new technology infrared-optimized telescope on that site. As part of these initiatives, UNAM became the second international member of the Association of Universities for Research in Astronomy (AURA), collaborated with the University of Texas in the construction of optical components for the Hobby-Eberly Telescope, and promoted studies for the construction of a Magellan-telescope clone at the SPM observatory. She also promoted the growth of the Institute's research branch located in Ensenada, Baja California, and the creation of a new branch located in the city of Morelia, Michoacán, which later evolved into UNAM's Instituto de Radioastronomía y Astrofísica. Koenigsberger holds a permanent position as professor and research scientist at UNAM's Instituto de Ciencias Físicas based in Cuernavaca, Morelos, is a member of the Sistema Nacional de Investigadores (SNI) at Level III. and a member of the International Astronomical Union (IAU). She served on the board of directors of the Association of Universities for Research in Astronomy (AURA) (1997-1999 and 2001-2007) and was a member of its Audit Committee from 2007 to 2016. Her research is devoted to the study of the structure and evolutionary processes in massive stars, particularly the effects caused by interactions in binary systems.

Recognition Koenigsberger is a member of the Mexican Academy of Sciences.

Selected publications Koenigsberger has published more than 120 research articles including:

Benítez-Llambay, Pablo; Masset, Frédéric; Koenigsberger, Gloria; Szulágyi, Judit (2015). "Planet heating prevents inward migration of planetary cores". Nature. 520 (7545): 63–65. arXiv:1510.01778. Bibcode:2015Natur.520...63B. doi:10.1038/nature14277. PMID 25832403. S2CID 4466971. Koenigsberger, Gloria; Morrell, Nidia; Hillier, D. John; Gamen, Roberto; Schneider, Fabian R. N.; González-Jiménez, Nicolás; Langer, Norbert; Barbá, Rodolfo (2014). "The Hd 5980 Multiple System: Masses and Evolutionary Status". The Astronomical Journal. 148 (4): 62. arXiv:1408.0556. Bibcode:2014AJ....148...62K. doi:10.1088/0004-6256/148/4/62. S2CID 118348677. Palate, M.; Koenigsberger, G.; Rauw, G.; Harrington, D.; Moreno, E. (2013). "Spectral modelling of theαVirginis (Spica) binary system". Astronomy & Astrophysics. 556: A49. arXiv:1307.1970. Bibcode:2013A&A...556A..49P. doi:10.1051/0004-6361/201321909. S2CID 53519054. Koenigsberger, G.; Moreno, E.; Koenigsberger, Gloria; Szulágyi, Judit (2013). "Tidal Flows in asynchronous binaries: The β-factor". EAS Publications Series. 64: 339–342. arXiv:1312.1372. Bibcode:2013EAS....64..339K. doi:10.1051/eas/1364047. S2CID 118387538. Flores, A.; Koenigsberger, G.; Cardona, O.; de la Cruz, L. (October 2011). "Wind Structure of the Wolf-Rayet Star EZ CMa = HD 50896". Revista Mexicana de Astronomía y Astrofísica. 47 (2): 261. Bibcode:2011RMxAA..47..261F. ISSN 0185-1101. Moreno, E.; Koenigsberger, G.; Harrington, D. M.; Szulágyi, Judit (2011). "Eccentric binaries". Astronomy & Astrophysics. 528: A48. arXiv:1102.4301. doi:10.1051/0004-6361/201015874. S2CID 59045830. Van Der Hucht, Karel A.; Koenigsberger, Gloria; Eenens, Philippe R. J. (1999). "Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies". Proceedings of the 193rd Symposium of the International Astronomical Union. San Francisco: Astronomical Society of the Pacific. ISBN 9781583810040.{{cite journal}}: CS1 maint: periodical has ISBN (link)

References

Illustrations

Gloria Suzanne Koenigsberger Horowitz illustration

Worked examples

Example 1 — a first encounter with Gloria Suzanne Koenigsberger Horowitz

Start with the simplest possible case. Write down what Gloria Suzanne Koenigsberger Horowitz 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 Gloria Suzanne Koenigsberger Horowitz 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 Gloria Suzanne Koenigsberger Horowitz 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 Gloria Suzanne Koenigsberger Horowitz

In research
Gloria Suzanne Koenigsberger Horowitz 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 Gloria Suzanne Koenigsberger Horowitz 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
Gloria Suzanne Koenigsberger Horowitz is common in secondary-school and first-year university syllabi. It links to neighbouring topics 20th-century Mexican physicists, 20th-century women physicists, 21st-century Mexican physicists, so understanding it makes those chapters shorter.
In everyday life
Look for Gloria Suzanne Koenigsberger Horowitz 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 Gloria Suzanne Koenigsberger Horowitz in 20 minutes

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

Frequently asked questions

What is Gloria Suzanne Koenigsberger Horowitz in simple terms?

Gloria Suzanne Koenigsberger Horowitz is a Mexican astrophysicist and professor working at the National Autonomous University of Mexico (UNAM). Her areas of expertise are in stellar spectroscopy, massive stars and binary interaction effects.

Why does Gloria Suzanne Koenigsberger Horowitz 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 Gloria Suzanne Koenigsberger Horowitz?

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 Gloria Suzanne Koenigsberger Horowitz.

Tags

  • 20th-century Mexican physicists
  • 20th-century women physicists
  • 21st-century Mexican physicists
  • 21st-century astronomers
  • Academic staff of the National Autonomous University of Mexico
  • Internet pioneers
  • Living people
  • Members of the Mexican Academy of Sciences
  • Mexican academic administrators
  • Mexican astronomers
  • Mexican scientists
  • Mexican women astronomers

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