Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-28T14:48:11.940Z Has data issue: false hasContentIssue false
  • English
  • Français

How Unusual are Stars with Planets?

Published online by Cambridge University Press:  19 September 2017

I. Neill Reid
I. Neill Reid*
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Comparative analysis of the parent stars of extrasolar planetary systems and the local disk population shows a strong trend for increasing frequency with increasing abundance. Approximately 4.5% of solar-abundance (−0.15 < [m/H] ≤ +0.15) stars have detectable planetary-mass companions.

Type
Extrasolar Planets
Information
Symposium - International Astronomical Union , Volume 213: Bioastronomy 2002: Life Among the stars , 2004 , pp. 51 - 54
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Gilliland, R., et al. 2001, ApJ, 545, L47 Google Scholar
Gonzalez, G. 1997, MNRAS, 285, 403 CrossRefGoogle Scholar
Haywood, M. 2002, MNRAS, in press Google Scholar
Marcy, G.M. 2004, this volume Google Scholar
Reid, I. N. 2002, PASP, 114, 306 CrossRefGoogle Scholar
Santos, N. C., Israelian, G., & Mayor, M. 2001, A&A, 373, 1019 Google Scholar
Tinney, C. E. 2004, this volume Google Scholar