Zobrazeno 1 - 10
of 152
pro vyhledávání: '"Hilmar W. Duerbeck"'
Autor:
Hilmar W. Duerbeck
Publikováno v:
Astronomische Nachrichten. 330:568-573
This article gives a brief overview of 400 years of research in the field of novae and related stars. Important objects, first applications of various observing techniques, and early ideas of the interpretation of phenomena are listed. Also, the hist
Autor:
Slavek M. Rucinski, Hilmar W. Duerbeck
Publikováno v:
The Astronomical Journal. 133:169-176
Radial velocity measurements and sine-curve fits to the orbital velocity variations are presented for 14 close binary stars, S Ant, TT Cet, TW Cet, AA Cet, RW Dor, UX Eri, YY Eri, BV Eri, CT Eri, SZ Hor, AD Phe, TY Pup, HI Pup, and TZ Pyx. All are do
Autor:
Hilmar W. Duerbeck, Slavek M. Rucinski
Publikováno v:
The Astronomical Journal. 132:1539-1546
Radial velocity measurements and sine-curve fits to the orbital velocity variations are presented for nine contact binaries: V1464 Aql, V759 Cen, DE Oct, MW Pav, BQ Phe, EL Aqr, SX Crv, VZ Lib, and GR Vir. For the first five of these, our observation
Autor:
Hilmar W. Duerbeck, Peter Beer
Publikováno v:
Journal of Astronomical History and Heritage. 9:93-98
Autor:
Hilmar W Duerbeck
Publikováno v:
Journal of Astronomical History and Heritage. :8-17
Autor:
Christiaan Sterken, Hilmar W Duerbeck
Publikováno v:
Journal of Astronomical History and Heritage. 7:25-33
Autor:
C. Sterken, Enrique Garcia-Melendo, Hilmar W. Duerbeck, Torben Arentoft, P. van Cauteren, Patricia Lampens
Publikováno v:
Astronomy & Astrophysics. 418:249-254
WX Eri is an eclipsing binary system for which one component was reported to show δ Scuti type pulsations with periods close to integer fractions of the orbital period. This makes it an interesting candidate for investigating the interaction be- twe
Autor:
Hilmar W. Duerbeck
4. Census of the Catalogue The catalogue contains information on 277 objects. 137 (50%) of them are stars whose outburst spectra or unambiguous mInImUm characteristics classify them as novae beyond doubt. 123 of them could be identified at minimum. 7
Autor:
Hilmar W. Duerbeck
Publikováno v:
Astronomische Nachrichten. 323:534-537
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 334:875-882
We present fits to 1–5 μm spectra of the dust shell around Sakurai's Object (V4334 Sgr) obtained over the period 1999 May to 2001 September, using the dusty modelling program. We find that the emission is consistent with carbon dust grains for whi