"Osiris"(HD209458b), an evaporating planet
Three transits of the planet orbiting the solar type star HD209458 were observed in the far UV at the wavelength
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A direct imaging search for wide (sub)stellar companions around rad-vel planet host stars
We present an overview of our ongoing systematic search for wide (sub)stellar companions around the stars known to host rad-vel
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A free-floating planet population in the Galaxy?
Most young low-mass stars are born as binary systems, and circumstellar disks have recently been observed around the individual components
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A Hot Saturn Planet Orbiting HD 88133, from the N2K Consortium
The N2K consortium is carrying out a distributed observing campaign with the Keck, Magellan and Subaru telescopes, as well as
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An Automated Search for Extrasolar Planet Transits
We are setting up a new search for transiting extrasolar planets using the 0.5m Automated Patrol Telescope at Siding Spring
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A New Transiting Extrasolar Giant Planet
We have measured radial velocities of a star, OGLE-TR-56, which shows a 1.2-day transit-like light curve found photometrically by Udalski
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A Planet Candidate in the Stellar Triple System HD178911
We report the detection of a low-mass companion orbiting the solar-type star HD178911B, the distant component of the stellar triple
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A planet orbiting the star Gliese 86
A 4MJ planet with a 15.8day orbital period has been detected from very precise radial velocity measurements with the CORALIE
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A Possible Hybrid Scenario for Gas Giant Planet Formation in Rings
The core-accretion mechanism for gas giant formation may be too slow to create all observed gas giant planets during reasonable
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Available Energy for Life on a Planet, with or without Stellar Radiation
The quest for life in the Universe is often affected by the free use of extrapolations of our phenomenological geocentric
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Bayesian Hypothesis Testing for Planet Detection
The past five years has seen a surge in research and innovative ideas for the imaging of extrasolar planets, particular
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Beyond the Cosmic Veil: Star and Planet Formation Research after SIRTF and NGST
How do planets form from circumstellar disks of gas and dust? What physical processes are responsible for determining the final
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Captain Cook, the Terrestrial Planet Finder and the Search for Extraterrestrial Intelligence
Over two hundred years ago Capt. James Cook sailed up Whitsunday Passage, just a few miles where we now sit,
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Chemical analysis of 8 recently discovered extra-solar planet host stars
We present the chemical analysis of a new set of stars known to harbor low mass companions, namely HD 1237,
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Choice of Observing Schedules for Astrometric Planet Searches
The Space Interferometry Mission (SIM) will make precise astrometric measurements that can be used to detect planets around nearby stars.
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Circumstellar Disks and Outer Planet Formation
The dust disk around Beta Pic must be produced by collision or by evaporation of orbiting Kuiper belt-like objects. Here
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Cosmological Constraints on Terrestrial Planet Formation
I attempt to piece together a consistent scenario based on current estimates of the evolution of the star formation rate
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Detection of a spectroscopic transit by the planet orbiting the star HD209458
We report the first detection of a planetary transit by spectroscopic measurements. We have detected the distortion of the stellar
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DID PLANET FORMATION BEGIN INSIDE PERSISTENT GASEOUS VORTICES?
We explore here the idea, reminiscent in some respect of Von Weizsacker's (1944) and Alfven's (1976) outmoded cosmogonies, that long-lived
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Disc-planet, planet-planet, and star-planet interactions during planet formation
In this article we present results from three on-going projects related to the formation of protoplanets in protostellar discs. We
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Dust to Dust: Evidence for Planet Formation?
We discuss the properties of several circumstellar debris disk systems imaged with the Hubble Space Telescope's Near Infrared Camera and
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Dynamical Model of Pulsar-Planet Systems
About two years ago, Wolszczan and Frail announced the detection of a possible planetary system consisting of two Earth-mass planets
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Exo-planet detection with the COROT space mission. I. A multi-transit detection criterion
We present a detection criterion for exo-planets to be used with the space mission COROT. This criterion is based on
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Extrasolar Planet Transit Light Curves and a Method to Select the Best Planet Candidates for Mass Follow-up
A unique analytical solution of planet and star parameters can be derived from an extrasolar planet transit light curve under
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