activity
19992002
collaborators

6 papers

astro-ph2002

Planetary system around Vega

N. Gorkavyi, T. Taidakova

We applied our earlier numerical method to compute the thermal emission from a dusty resonant structure around Vega and compared the new observational evidence for a ring arc at 95…

astro-ph2000

Indicator of Exo-Solar Planet(s) in the Circumstellar Disk Around Beta Pictoris

Nick Gorkavyi, Sara Heap, Leonid Ozernoy +2

Our efficient numerical approach has been applied to modeling the asymmetric circumstellar dust disk around Beta Pictoris as observed with the HST/STIS. We present a new model on t…

astro-ph2000

Resonant Gaps in the Scattered Cometary Population of the Trans-Neptunian Region

Tanya Taidakova, Leonid M. Ozernoy, Nick N. Gorkavyi

Our numerical simulations of the Edgeworth-Kuiper belt objects gravitationally scattered by the four giant planets accounting for mean motion resonances reveal numerous resonant ga…

astro-ph2000

Distribution of dust from Kuiper belt objects

Nick N. Gorkavyi, Leonid M. Ozernoy, Tanya Taidakova +1

(Abridged) Using an efficient computational approach, we have reconstructed the structure of the dust cloud in the Solar system between 0.5 and 100 AU produced by the Kuiper belt o…

astro-ph2000

Orbital Motion of Resonant Clumps in Dusty Circumstellar Disks as a Signature of an Embedded Planet

Nick N. Gorkavyi, Leonid M. Ozernoy, John C. Mather +1

We have applied a powerful numerical approach to compute, with a high resolution, the structure of dusty circumstellar disks with embedded planets. We emphasize some testable impli…

astro-ph1999

The NGST and the zodiacal light in the Solar system

Nick Gorkavyi, Leonid Ozernoy, John Mather +1

We develop a physical model of the zodiacal cloud incorporating the real dust sources of asteroidal, cometary, and kuiperoidal origin. Using the inferred distribution of the zodiac…