| |
Barwig, H. |
| Volume |
Paper Title |
Page Number |
Authors |
| 56 |
The HST Observations of IP Pegasi: A First Look at the Data |
259 |
Baptista, R.; Horne, K.; Eracleous, M.; Barwig, H.; Long, K.; Mantel, K.-H.; Marsh, T. R.; Polidan, R. S.; Raymond, J. C.; Roginson, E. L.; Rutten, R. G. M.; Shafter, A. W.; Szkody, P.; Wade, R. A.; Wood, J.; Zhang, E.-H. |
| 96 |
Is GP Coin a true AM CVn system? |
313 |
Ulla, A.; Mantel, K.-H.; Barwig, H.; La Dous, C.; Sabau, L.; Goodrich, R. W. |
| 152 |
The Impact of Fiber Optics on Photometry: the Design of Two High-Speed Multichannel Instruments |
320 |
Barwig, H.; Mantel, K. H.; Kiesewetter, S. |
| 251 |
High Resolution X-ray Spectroscopy of the Magnetic Cataclysmic Variables AM Her and PQ Gem with the Chandra LETGS |
344 |
Burwitz, V.; Haberl, F.; Predehl, P.; Reinsch, K.; Barwig, H. |
| 261 |
Detection of spiral structure in the quiescent accretion disk of IP Pegasi |
513 |
Neustroev, V. V.; Borisov, N. V.; Barwig, H.; Bobinger, A.; Mantel, K. H.; šimíc, D.; Wolf, S. |
| 310 |
Variable Star Monitoring in Local Group Dwarf Irregular Galaxies |
70 |
Snigula, J.; Goessl, C.; Hopp, U.; Barwig, H. |
| 330 |
Four-Component Model of the Auto-Correlation Function of AM Her Based on a CHANDRA Observation |
407 |
Andronov, I.L.; Burwitz, V.; Reinsch, K.; Barwig, H.; Chinarova, L.L.; Kolesnikov, S.V.; Shakhovskoy, N.M.; Hambaryan, V.; Beuermann, K.; Yukhanov, D.A. |
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