Paper Title |
Page |
Authors |
|
| |
Introductory review: Some general problems concerning RCB stars |
3 |
Feast, M. W. |
R Coronae Borealis stars: current status of the observational data |
13 |
Cottrell, P. L. |
Model atmospheres of cool hydrogen-deficient carbon stars |
27 |
Gustafsson, B.; Asplund, M. |
Are the declines of R Coronae Borealis stars caused by super- Eddington luminosities? |
39 |
Asplund, M.; Gustafsson, B. |
Surface composition of the RCB stars - refinement of a few mere facts |
43 |
Rao, N. K.; Lambert, D. L. |
A non-LTE investigation of carbon in R Coronae Borealis stars |
57 |
Asplund, M.; Ryde, N. A. E. |
Hydrogen-deficient nature of Z UMi |
58 |
Goswami, A.; Rao, N. K.; Gonzalez, G.; Lambert, D. L. |
Spectrum of S APS at deep minimum |
59 |
Rao, N. K.; Goswami, A.; Smith, V. V.; Lambert, D. L. |
R CR B pulsation and mass loss |
60 |
Rao, N. K.; Lambert, D. L. |
Observational properties of dust shells of R Coronae Borealis stars |
63 |
Clayton, G. |
Chemistry and thermodynamics of the nucleation in R CrB star shells |
69 |
Goeres, A. |
Shock-induced condensation in R CrB stars |
83 |
Woitke, P.; Goeres, A.; Sedlmayr, E. |
Pulsationally induced dust formation in evolved stars |
87 |
Lafon, J.-P. J. |
What causes the R Corona Borealis type minimum: dust cloud or dust shell? |
91 |
Rosenbush, A. E. |
Long-term photometry of R Coronae Borealis (RCB) stars |
95 |
Cottrell, P. L.; Gilmore, A. G.; Kilmartin, P. M.; Pooley, D. J.; Lawson, W. A. |
On the inter-fade periods of R CrB type variables |
96 |
Jurcsik, J. |
Short-time low-amplitude fadings in R CrB and XX Cam-a rapid dust-producing phenomenon? |
97 |
Zhilyaev, B.; Totochava, A. G. |
The mathematically strict analysis of the extinction curves of the RCB 98 stars |
98 |
Zubko, W. |
Wolf-Rayet central stars of planetary nebulae |
101 |
Tylenda, R. |
Wolf-Rayet stars and stellar winds |
111 |
Hillier, D. J. |
Wolf-Rayet stars of high and low mass |
127 |
Hamann, W.-R. |
Non-LTE spectroscopic analysis of the wind of the central star of NGC 6543 |
141 |
de Koter, A.; Hubeny, I.; Heap, S. R.; Lanz, T. |
A method for the direct determination of the wind electron temperature of WC10 central stars of planetary nebulae |
145 |
De Marco, O.; Storey, P. J.; Barlow, M. J. |
A quantitative analysis of the [WCL] star CPD-56 Degrees 8032 |
149 |
Crowther, P. A.; De Marco, O.; Storey, P. J.; Barlow, M. J. |
Spectral analyses of late-type WR central stars: upper limits for the hydrogen abundance |
150 |
Leuenhagen, U. |
A 3000-d visual light curve for the [WC11] star CPD-56 Degrees 8032 (V837 Ara) |
151 |
Lawson, W. A.; Jones, A. F. |
Surface properties of extreme helium stars |
152 |
Jeffery, C. S. |
MV SGR - the emission line spectrum |
167 |
Pandey, G.; Rao, N. K.; Lambert, D. L. |
Spectral variations of DY CEN |
171 |
Giridhar, S.; Rao, N. K.; Lambert, D. L. |
Spectral analysis of the extreme helium star LSS 3184 |
172 |
Drilling, J. S.; Jeffery, C. S.; Heber, U. |
A spectral analysis of the H-deficient star HD144941 |
173 |
Harrison, P. M.; Jeffery, C. S. |
NLTE analysis of the extreme helium star HD 160641 |
174 |
Rauch, T. |
Spectrum synthesis of type IA SNe |
175 |
Hauschildt, P. H.; Baron, E.; Nugent, P.; Branch, D. |
Stellar wind and elemental segregation |
179 |
Hunger, K.; Groote, D.; Heber, U. |
He-rich stars and the fading of radiatively driven winds |
185 |
Babel, J. |
X-ray emission from magnetically confined winds |
189 |
Babel, J.; Montmerle, T. |
Observations and models of H-deficient planetary nebulae |
193 |
Harrington, J. P. |
The planetary nebulae K1-27 and LoTr4 and their central stars |
205 |
Koppen, J.; Rauch, T.; Werner, K. |
[WR] nuclei of planetary nebulae: inferences from statistical studies of the nebulae |
209 |
Gorny, S. K.; Stasinska, G. |
The planetary nebulae of PG 1159 stars - clues to their evolutionary history |
213 |
Napiwotzki, R.; Haas, S.; Schonberner, D. |
Morphology of the planetary nebula Lo4 |
217 |
Kohoutek, L. |
CPD -56 Degrees 8032: a very low-excitation planetary nebula |
219 |
Kohoutek, L. |
HST narrow-band imaging and UV spectrophotometry of planetary nebulae in the Magellanic Clouds |
220 |
Vassiliadis, E.; Dopita, M. A.; Meatheringham, S. J.; Bohlin, R. C.; Ford, H. C.; Harrington, J. P.; Wood, P. R.; Stecher, T. P.; Maran, S. P. |
The statistics and classification of hydrogen-deficient white dwarfs: ten years post-Mysore |
223 |
Sion, E. M. |
Helium-rich stars from the HS, PG and KPD surveys |
241 |
Heber, U.; Dreizler, S.; Werner, K.; Engels, D.; Hagen, H.-J. |
Proper motions of the hot subdwarfs: observations and population tests |
245 |
Thejll, P.; Flynn, C.; The CAMC Team |
Fully line-blanketed NLTE model atmospheres for hot hydrogen-deficient stars |
249 |
Hubeny, I.; Lanz, T. |
The role of blanketing by iron-group elements in sdO stars atmospheres |
261 |
Haas, S. |
Solution of the Balmer line problem |
265 |
Werner, K. |
Sphericity effects in helium rich NLTE model atmospheres |
266 |
Kubat, J. |
PG 1159 stars |
267 |
Werner, K.; Dreizler, S.; Heber, U.; Rauch, T. |
Spectral analysis of hot helium-rich white dwarfs |
281 |
Dreizler, S.; Werner, K. |
The DB and DBA white dwarfs: epitomes of hydrogen-deficient stars |
295 |
Beauchamp, A.; Wesemael, F.; Bergeron, P.; Liebert, J.; Saffer, R. A. |
AM CVn binaries - will they evolve into DB white dwarfs? |
309 |
Solheim, J. E. |
Is GP Coin a true AM CVn system? |
313 |
Ulla, A.; Mantel, K.-H.; Barwig, H.; La Dous, C.; Sabau, L.; Goodrich, R. W. |
NLTE spectral analysis of helium-rich sdO stars from the southern HK survey |
317 |
Drilling, J. S.; Napiwotzki, R.; Dreizler, S.; Heber, U.; Beers, T. C. |
Analysis of IR photometry for sdO stars |
318 |
Ulla, A.; Thejll, P. |
Observations of PG 1159 stars with the Hopkins Ultraviolet Telescope |
319 |
Kruk, J. W.; Werner, K. |
Is the transformation of atmospheres by diffusion possible? |
320 |
Unglaub, K.; Bues, I. |
GD358 and the role of hydrogen in DB evolution |
321 |
Provencal, J. L.; Shipman, H. L. |
The instability strip of the pulsating DB (V777 Her) white dwarfs: a preliminary view in the optical |
322 |
Wesemael, F.; Beauchamp, A.; Bergeron, P.; Fontaine, G.; Saffer, R. A.; Liebert, J. |
Analysis of the helium-rich magnetic white dwarf GD 1702 |
323 |
Fey, W.; Bues, I. |
L745-46A: hydrogen and metal abundances in a He-rich white dwarf |
324 |
Koester, D.; Allard, N. F. |
Molecules in the atmospheres of helium-rich very cool white Dwarfs |
325 |
Aslan, T.; Bues, I.; Karl-Dietze, L. |
The story of PG SGE |
329 |
Kipper, T. |
On the evolution and mass of FG SGE |
341 |
Blocker, T.; Schonberner, D. |
High resolution spectra of FG SGE during the 1992 and 1994 deep minima |
345 |
Smith, V. V.; Gonzalez, G.; Rao, N. K. |
The observational characterization of hydrogen-deficient carbon stars as pulsating stars |
349 |
Lawson, W. A.; Kilkenny, D. |
Linear models for hydrogen-deficient star pulsations |
361 |
Saio, H. |
Small amplitude variations in XX Cam and three other northern hemisphere RCrB stars |
374 |
Weiss, A.; Olson, E. G.; Fried, R. |
Nonlinear radial pulsation models for hydrogen-deficient stars |
375 |
Fadeyev, Yu. A. |
A nonlinear radial pulsation model for the extreme helium star V652 387 HER (BD+13 Degrees 3224) |
387 |
Fadeyev, Yu. A.; Lynas-Gray, A. E. |
Pulsations and mass loss of hydrogen-deficient carbon stars |
391 |
Dorfi, E.; Feuchtinger, M. U. |
Ultraviolet light curves for pulsating helium stars |
395 |
Hill, P. W.; Jeffery, C. S. |
A radial velocity curve for pulsating helium star LSS3184 |
396 |
Jeffery, C. S.; Hill, N. C. |
Asteroseismology of PG1159 stars |
397 |
Vauclair, G. |
On the origin of R CrB and other hydrogen-deficient stars |
409 |
Iben, I.; Tutukov, A. V.; Yungelson, L. R. |
The progenitors of hydrogen-deficient supernovae |
419 |
Podsiadlowski, P. |
How are hydrogen-deficient stars formed? |
433 |
Schonberner, D. |
Observational evidence for evolutionary links |
443 |
Lambert, D. |
Basic data on hydrogen-deficient stars |
461 |
Drilling, J. S. |
A catalogue of hydrogen-deficient stars |
471 |
Jeffery, C. S.; Heber, U.; Hill, P. W.; Dreizler, S.; Drilling, J. S.; Lawson, W. A.; Leuenhagen, U.; Werner, K. |