New debris disks around nearby main-sequence stars : Impact on the direct detection of planets
- Author
- BEICHMAN, C. A1 ; BRYDEN, G2 ; LUNINE, J. I3 ; FISCHER, D. A4 ; MARCY, G. W5 ; GREAVES, J. S6 ; WYATT, M. C7 ; HOLLAND, W. S8 ; DENT, W. R. F8 ; STAPELFELDT, K. R2 ; GAUTIER, T. N2 ; GROGAN, K2 ; SHAO, M2 ; VELUSAMY, T2 ; LAWLER, S. M1 ; BLAYLOCK, M3 ; RIEKE, G. H3
[1] Michelson Science Center, California Institute of Technology, 770 South Wilson Avenue, Pasadena, CA 91125, United States
[2] Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, United States
[3] Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, United States
[4] Department of Physics and Astronomy, San Francisco State University, San Francisco, CA 94132, United States
[5] Department of Astronomy, University of California, Berkeley, CA 94720, United States
[6] School of Physics and Astronomy, University of St. Andrews, North Haugh, St. Andrews KY16 9SS, United Kingdom
[7] Institute of Astronomy, University of Cambridge, Cambridge CB3 0HA, United Kingdom
[8] UK Astronomy Technology Centre, Royal Observatory, Edinburgh EH9 3HJ, United Kingdom - Source
The Astrophysical journal. 2006, Vol 652, Num 2, pp 1674-1693, 20 p ; 1 ; ref : 84 ref
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- K-uiper Belt circumstellar matter infrared: stars
- Keyword (fr)
- Etoile IR Etoile proche Etoile séquence principale Matière circumstellaire Planète
- Keyword (en)
- Infrared star Nearby stars Main sequence stars Circumstellar matter Planets
- Keyword (es)
- Estrella IR
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18364734
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1086/508449 
https://dx.doi.org/10.1086/508449
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