Search Results - "Schoembs, R."

Periodic variations in PHL 227 by Haefner, R., Schoembs, R.

“…Spectroscopic and photometric observations of the recently discovered UX UMa star PHL 227 are presented. An orbital period of 0.1356±0.0006 day results from…”
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The ephemeris and variations of the accretion disc radius in IP Pegasi by Wood, Janet H., Marsh, T. R., Robinson, E. L., Stiening, R. F., Horne, Keith, Stover, R. J., Schoembs, R., Allen, S. L., Bond, Howard E., Jones, D. H. P., Grauer, Albert D., Ciardullo, Robin

“…We present timings of 37 previously unpublished eclipses of the dwarf nova IP Pegasi, obtained in 1986 through to 1988, and combine these with earlier…”
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Dwarf novae in outburst: simultaneous ultraviolet and optical observations of UZ Serpentis, RX Andromedae and AH Herculis by Verbunt, F., Pringle, J. E., Wade, R. A., Echevarria, J., Jones, D. H. P., Argyle, R. W., Schwarzenberg-Czerny, A., la Dous, C., Schoembs, R.

“…We present spectroscopic and photometric observations in the optical and ultraviolet wavelength regions made during outbursts of the three dwarf novae UZ…”
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Spectroscopy of CN Orionis by Mantel, K. H., Barwig, H., Haefner, R., Schoembs, R.

“…Spectroscopic observations of the dwarf nova CN Orionis during two outbursts and a minimum phase have been analyzed. Periodic variations of the absorption…”
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Spectroscopy and optical/IR photometry of the cataclysmic variable CPD ― 48°1577 by WARGAU, W, BRUCH, A, DRECHSEL, H, RAHE, J, SCHOEMBS, R

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Dwarf novae in outburst: simultaneous ultraviolet and optical observations of RU Pegasi and TZ Persei by la Dous, C., Verbunt, F., Schoembs, R., Argyle, R. W., Jones, D. H. P., Schwarzenberg–Czerny, A., Hassall, B. J. M., Pringle, J. E., Wade, R. A.

“…We present ultraviolet and optical observations of the dwarf novae RU Peg and TZ Per during decline from outburst. In both systems the flux drops…”
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Spectroscopy and optical/IR photometry of the cataclysmic variable CPD -48 deg 1577 by WARGAU, W, Drechsel, H, Rahe, J, Bruch, A, SCHOEMBS, R

“…The photometric variability of CPD -48 deg 1577 in the optical and IR ranges is discussed. The structure and variation of prominent emission line profiles are…”
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