Zobrazeno 1 - 10
of 101
pro vyhledávání: '"B. Peschke"'
Publikováno v:
DMW - Deutsche Medizinische Wochenschrift. 121:1440-1445
Autor:
T. Kostiuk, D. J. Lien, H. U. Käufl, D. J. Osip, Eberhard Grün, Yanga R. Fernandez, M. F. A'Hearn, Carey M. Lisse, R. G. Walker, S. B. Peschke
Publikováno v:
Icarus. 171:444-462
We present the characteristics of the dust comae of two comets, 126P/IRAS, a member of the Halley family (a near-isotropic comet), and 2P/Encke, an ecliptic comet. We have primarily used mid- and far-infrared data obtained by the ISOPHOT instrument a
Autor:
A. B. Schultz, Varoujan Gorjian, Carey M. Lisse, Michael E. Ressler, S. B. Peschke, Yanga R. Fernandez, B. Golisch, Damian J. Christian, S. G. Djorgovski, C. Kaminski
Publikováno v:
The Astrophysical Journal. 570:779-784
We have discovered an extremely red object, LSF 1, located 7'' southwest (P.A. 217°) of the bright spectroscopic binary system HD 155826. Originally reported by IRAS as one source detected at 12-60 μm, and found as a single 6-25 μm source of simil
Autor:
S. B. Peschke, Humberto Campins, T. Y. Brooke, Manfred Stickel, Eberhard Grün, H. U. Keller, J. Crovisier, M. Solc, V. Vanysek, John C. Zarnecki, David J. Osip, Mark V. Sykes, R. F. Knacke, Dietrich Lemke, Carey M. Lisse, Michael Müller, I. Heinrichsen, Philippe Lamy, Ch. Leinert, Harald Krüger, H. Boehnhardt, Martha S. Hanner, T. G. Muller, C. Delahodde
Publikováno v:
Scopus-Elsevier
Comet Hale-Bopp was observed five times with ISOPHOT, the photometer on board ESA's Infrared Space Observatory (ISO) between 4.6 and 2.8 AU. Each time, broadband photometry was performed using 4 different detectors, 5 apertures and 10 filters coverin
Autor:
Philippe Lamy, Michael F. A'Hearn, Carey M. Lisse, Harold A. Weaver, Theodor Kostiuk, H. Ulrich Kaufl, Yanga R. Fernandez, Sibylle B Peschke, Timothy A. Livengood
Publikováno v:
Icarus. 147:145-160
We report a new study of the nucleus of Comet 2P/Encke, which the CONTOUR spacecraft is scheduled to encounter in November 2003. During the comet's close approach to Earth in July 1997, we measured the mid-infrared thermal and optical scattered conti
Autor:
Michael F. A'Hearn, Aditya Dayal, Yanga R. Fernandez, S. B. Peschke, Joseph L. Hora, Eberhard Grün, H. U. Kaufl, Michael E. Ressler, Giovanni G. Fazio, Timothy A. Livengood, William F. Hoffmann, Martha S. Hanner, Theodor Kostiuk, Carey M. Lisse, Lynne K. Deutsch
Publikováno v:
Earth, Moon, and Planets. 78:251-257
We present infrared imaging and photometry of the bright, giant comet C/1995 O1 (Hale-Bopp). The comet was observed in an extended infrared and optical observing campaign in 1996–1997. The infrared morphology of the comet was observed to change fro
Autor:
A. Fiedler, Richard M. West, S. B. Peschke, G. P. Tozzi, H. Boehnhardt, Rita Schulz, K. Birkle, G. Schwehm, Nicolas Thomas, Laurent Jorda, Heike Rauer
Publikováno v:
Earth, Moon, and Planets. 78:179-187
In 1996 comet Hale-Bopp exhibited a porcupine-like coma with straight jets of dust emission from several active regions on the nucleus. The multi-jet coma geometry developed during the first half of 1996. While the jet orientation remained almost con
Autor:
Ingolf Heinrichsen, Ch. Leinert, Eberhard Grün, Roger F. Knacke, Hermann Böhnhardt, John C. Zarnecki, S. B. Peschke, David J. Osip, Humberto Campins, Dietrich Lemke, Manfred Stickel, Carey M. Lisse, Martha S. Hanner, Mark V. Sykes
Publikováno v:
Earth, Moon, and Planets. 78:299-304
Comet Hale-Bopp has been observed five times with ISOPHOT, the photometer on board the Infrared Space Observatory (ISO), four times before its perihelion passage at heliocentric distances of 4.92, 4.58, 2.93 and 2.81 AU, and at 3.91 AU postperihelion
Publikováno v:
ChemInform. 23
Publikováno v:
ChemInform. 27