Search Results - "Mantel, K. H"

The photometric and spectroscopic variability of 1329-294 by HAEFNER, R, BARWIG, H, MANTEL, K.-H

“…Photometric and spectroscopic observations of the poorly documented cataclysmic variable 1329-294 are presented. No definite period neither on a long nor on a…”
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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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IP Pegasi: Investigation of the accretion disk structure. Searching evidences for spiral shocks in the quiescent accretion disk by Neustroev, V. V, Borisov, N. V, Barwig, H, Bobinger, A, Mantel, K. H, Simic, D, Wolf, S

“…Astron.Astrophys. 393 (2002) 239-250 We present the results of spectral investigations of the cataclysmic variable IP Peg in quiescence. Optical spectra…”
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Detection of spiral structure of the quiescent accretion disk of IP Pegasi by Neustroev, V. V, Borisov, N. V, Barwig, H, Bobinger, A, Mantel, K. H, Simic, D, Wolf, S

“…We present the results of the spectral investigations of IP Peg in quiescence. Optical spectra obtained on 6-m telescope at the Special Astrophysical…”
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RXJ0806.3+1527: a double degenerate binary with the shortest known orbital period (321s) by Israel, G. L, Hummel, W, Covino, S, Campana, S, Appenzeller, I, Gassler, W, Mantel, K. -H, Marconi, G, Mauche, C. W, Munari, U, Negueruela, I, Nicklas, H, Rupprecht, G, Smart, R. L, Stahl, O, Stella, L

“…We carried out optical observations of the field of the X-ray pulsator RXJ0806.3+1527. A blue V=21.1 star was found to be the only object consistent with the…”
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Polars -- multisite emission -- multiwavelength observation by Schwope, Axel D, Beuermann, K, Buckley, D. A. H, Ciardi, D, Cropper, M, Horne, K, Howell, S, Mantel, K. -H, Metzner, A, O'Brien, K, Schwarz, R, Sirk, M, Steeghs, D, Still, M, Thomas, H. -C

“…We review the main observational characteristics of AM Herculis stars (polars) at X-ray, EUV, UV, IR and optical wavelengths. Particular emphasis is given to…”
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