An Estimate of the Age Distribution of Terrestrial Planets in the Universe: Quantifying Metallicity as a Selection Effect
- 1 June 2001
- Vol. 151 (2) , 307-313
- https://doi.org/10.1006/icar.2001.6607
Abstract
No abstract availableKeywords
All Related Versions
Funding Information
- Australian Research Council
This publication has 31 references indexed in Scilit:
- Planetary Companions to the Metal‐rich Stars BD −10o3166 and HD 52265The Astrophysical Journal, 2000
- A Lack of Planets in 47 Tucanae from a [ITAL]Hubble Space Telescope[/ITAL] SearchThe Astrophysical Journal, 2000
- Models of the in Situ Formation of Detected Extrasolar Giant Planets,,Icarus, 2000
- Is the Sun anomalous?Astronomy and Geophysics, 1999
- Disappearance of stellar debris disks around main-sequence stars after 400 million yearsNature, 1999
- Structure and Evolution of Nearby Stars with Planets. I. Short‐Period SystemsThe Astrophysical Journal, 1999
- Possible Stellar Metallicity Enhancements from the Accretion of PlanetsThe Astrophysical Journal, 1997
- The stellar metallicity--giant planet connectionMonthly Notices of the Royal Astronomical Society, 1997
- Proximity of Jupiter-Like Planets to Low-Mass StarsScience, 1995
- A survey of proper-motion stars. VII - The halo metallicity distribution functionThe Astronomical Journal, 1988