Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Dermott, S."'
Publikováno v:
Astrophysical Journal, 2015, Volume 811, Number 1
We have performed detailed dynamical modeling of the structure of a faint dust band observed in coadded IRAS data at an ecliptic latitude of 17$^{\circ}$ that convincingly demonstrates that it is the result of a relatively recent (significantly less
Externí odkaz:
http://arxiv.org/abs/1510.00615
Autor:
Krüger, Harald, Dikarev, V., Anweiler, B., Dermott, S. F., Graps, A. L., Gruen, E., Gustafson, B. A., Hamilton, D. P., Hanner, M. S., Horanyi, M., Kissel, J., Linkert, D., Linkert, G., Mann, I., McDonnell, J. A. M., Morfill, G. E., Polanskey, C., Schwehm, G., Srama, R.
The Ulysses spacecraft has been orbiting the Sun on a highly inclined ellipse since it encountered Jupiter in February 1992. Since then it made almost three revolutions about the Sun. Here we report on the final three years of data taken by the on-bo
Externí odkaz:
http://arxiv.org/abs/0908.1279
Autor:
Krüger, Harald, Bindschadler, D., Dermott, S. F., Graps, A. L., Gruen, E., Gustafson, B. A., Hamilton, D. P., Hanner, M. S., Horanyi, M., Kissel, J., Linkert, D., Linkert, G., Mann, I., McDonnell, J. A. M., Moissl, R., Morfill, G. E., Polanskey, C., Roy, M., Schwehm, G., Srama, R.
The Galileo spacecraft was orbiting Jupiter between Dec 1995 and Sep 2003. The Galileo dust detector monitored the jovian dust environment between about 2 and 370 R_J (jovian radius R_J = 71492 km). We present data from the Galileo dust instrument fo
Externí odkaz:
http://arxiv.org/abs/0908.1051
Autor:
Krüger, H., Grün, E., Graps, A., Bindschadler, D., Dermott, S., Fechtig, H., Gustason, B. A., Hamilton, D. P., Hanner, M. S., Horányi, M., Kissel, J., Lindblad, B. A., Linkert, D., Linkert, G., Mann, I., McDonnell, J. A. M., Morfill, G. E., Planskey, C., Schwehm, G., Srama, R., Zook, H. A.
The dust detector system onboard Galileo records dust impacts in circumjovian space since the spacecraft has been injected into a bound orbit about Jupiter in December 1995. This is the sixth in a series of papers dedicated to presenting Galileo and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0107052
Autor:
Krüger, H., Grün, E., Landgraf, M., Dermott, S., Fechtig, H., Gustafson, B. A., Hamilton, D. P., Hanner, M. S., Horányi, M., Kissel, J., Lindblad, B. A., Linkert, D., Linkert, G., Mann, I., McDonnell, J. A. M., Morfill, G. E., Polanskey, C., Schwehm, G., Srama, R., Zook, H. A.
The Ulysses spacecraft is orbiting the Sun on a highly inclined ellipse ($ i = 79^{\circ}$, perihelion distance 1.3 AU, aphelion distance 5.4 AU). Between January 1996 and December 1999 the spacecraft was beyond 3 AU from the Sun and crossed the ecli
Externí odkaz:
http://arxiv.org/abs/astro-ph/0106322
Recent observations of the size-frequency distribution of zodiacal cloud particles obtained from the cratering record on the LDEF satellite (Love and Brownlee 1993) reveal a significant large particle population (100 micron diameter or greater) near
Externí odkaz:
http://arxiv.org/abs/astro-ph/0005286
Autor:
Telesco, C. M., Fisher, R. S., Pina, R. K., Knacke, R. F., Dermott, S. F., Wyatt, M. C., Grogan, K., Holmes, E. K., Ghez, A. M., Prato, L., Hartmann, L. W., Jayawardhana, R.
We present new 10.8 and 18.2 micron images of HR 4796A, a young A0V star that was recently discovered to have a spectacular, nearly edge-on, circumstellar disk prominent at ~20 microns (Jayawardhana et al. 1998; Koerner et al. 1998). These new images
Externí odkaz:
http://arxiv.org/abs/astro-ph/9909363
Autor:
Wyatt, M. C., Dermott, S. F., Telesco, C. M., Fisher, R. S., Grogan, K., Holmes, E. K., Pina, R. K.
Publikováno v:
Astrophys.J.527:918-944,1999
Recent images of the disks of dust around the young stars HR 4796A and Fomalhaut show, in each case, a double-lobed feature that may be asymmetric (one lobe may be brighter than the other). A symmetric double-lobed structure is that expected from a d
Externí odkaz:
http://arxiv.org/abs/astro-ph/9908267
Autor:
Krüger, H., Grün, E., Hamilton, D. P., Baguhl, M., Dermott, S., Fechtig, H., Gustafson, B. A., Hanner, M. S., Horányi, M., Kissel, J., Lindblad, B. A., Linkert, D., Linkert, G., Mann, I., McDonnell, J. A. M., Morfill, G. E., Polanskey, C., Riemann, R., Schwehm, G., Srama, R., Zook, H. A.
Between Jan 1993 and Dec 1995 the Galileo spacecraft traversed interplanetary space between Earth and Jupiter and arrived at Jupiter on 7 Dec 1995. The dust instrument onboard was operating during most of the time. A relatively constant impact rate o
Externí odkaz:
http://arxiv.org/abs/astro-ph/9809318
Autor:
Krüger, H., Grün, E., Landgraf, M., Baguhl, M., Dermott, S., Fechtig, H., Gustafson, B. A., Hamilton, D. P., Hanner, M. S., Horányi, M., Kissel, J., Lindblad, B. A., Linkert, D., Linkert, G., Mann, I., McDonnell, J. A. M., Morfill, G. E., Polanskey, C., Schwehm, G., Srama, R., Zook, H. A.
The Ulysses spacecraft is orbiting the Sun on a highly inclined ellipse ($i = 79^{\circ}$). After its Jupiter flyby in 1992 at a heliocentric distance of 5.4 AU, the spacecraft reapproached the inner solar system, flew over the Sun's south polar regi
Externí odkaz:
http://arxiv.org/abs/astro-ph/9809133