A&A press release: German high-school students involved in an astronomical [..] (5 November 2009)
- Published on 02 November 2009
A&A press release
Released on November 5th, 2009
German high-school students involved in an astronomical research
project on cataclysmic variable stars
Based on the article:
“A long-term optical and X-ray ephemeris of the polar EK Ursae Majoris” by K. Beuermann et al.
To be published in Astronomy & Astrophysics
Astronomy & Astrophysics
publishes the results of an
unusual research project, by a team involving German high-school
students. They present an accurate, long-term ephemeris of the
cataclysmic variable EK Ursae Majoris, obtained using a professional
Cataclysmic variable research is a field where the contributions of small telescopes has a long tradition. Cataclysmic variables are extremely close binary systems containing a low-mass star whose material is being stripped off by the gravitational pull of a white dwarf companion. Due to the transfer of matter between the stars, these systems vary dramatically in brightness on timescales in the whole range between seconds and years. This largely unpredictable variability makes them ideal targets for school projects, particularly since professional observatories are generally unable to provide enough observation time for regular monitoring.
An accurate ephemeris is needed to keep track of the orbital motions of the two stars, but none was available because EK UMa is faint in the optical range and requires a long-term observation of the light variations. The strong magnetic field of the white dwarf turns the light of the hot matter striking the surface of the white dwarf into two “lighthouse” beams. By measuring the times of the minimum between the beams, the group was able to determine an orbital period accurate enough to keep track of the eclipse that took place in 1985, over 100 000 cycles earlier. By combining their own measurements with those made by the Einstein, ROSAT, and EUVE satellites, they estimated the orbital period over 137 000 cycles to an accuracy of a tenth of a millisecond. Surprisingly, the orbital period is extremely stable, although the period of such very close binaries is expected to vary due to the presence of third bodies and magnetic activity cycles on the companion star.
The pupils were involved in the various tasks of the research project: observations, analysis of the CCD images, production and interpretation of light curves, and access to the archival satellite data. They participated in all the steps of a real research program, from initial observations to the publication process, and the result they obtained bears scientific significance. Team leader K. Beuermann concluded: “Although it is fun to perform one's own remote observations with a professional telescope from the comfort of a normal school classroom, it is even more satisfying to be involved in a project that provides new and publishable results rather than to perform experiments with predictable outcomes.”
Fig. 1 - From the left: Klaus Beuermann (group leader), Jens Diese (back,teacher), and the high-school students Joshua Zachmann (front), Alexander-Maria Ploch (back), Sang Paik (front). JD, JZ, and AMP are from the Max-Planck-Gymnasium, SP is from the Felix-Klein-Gymnasium. Team members Axel Schwope and Frederic Hessman are not in the picture.
 The team includes a secondary school physics teacher, Jens Diese, three 12th grade pupils, Sang Paik, Alexander-Maria Ploch, and Joschua Zachmann, and three professional astronomers, Klaus Beuermann, Frederic Hessman (Univ. Göttingen), and Axel Schwope (AIP, Postdam).
 Max-Planck-Gymnasium/Göttingen, Felix-Klein-Gymnasium/Göttingen
 The telescope used for this project is operated by the Univ. of Göttingen, the Univ. of Texas at Austin, and the South African Astron. Obs.
A long-term optical and X-ray ephemeris of the polar EK Ursae Majoris, by K. Beuermann, J. Diese, S. Paik, A. Ploch, J. Zachmann, A.D. Schwope, and F.V. Hessman.
To be published in Astronomy & Astrophysics,
Full article available in PDF format
Universität Göttingen, Institut für Astrophysik
37077 Göttingen, Germany
Email: beuermann (at) astro.physik.uni-goettingen.de
Phone: +49 5508 1248
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© Astronomy & Astrophysics 2009