M Stars as Targets for Terrestrial Exoplanet Searches And Biosignature Detection-Reference-Cited by-同舟云学术

M Stars as Targets for Terrestrial Exoplanet Searches And Biosignature Detection

Published:2007-02 Issue:1 Volume:7 Page:85-166
ISSN:1531-1074
Container-title:Astrobiology
language:en
Short-container-title:Astrobiology

Author:

Scalo John¹,Kaltenegger Lisa²,Segura Antígona³,Fridlund Malcolm⁴,Ribas Ignasi⁵⁶,Kulikov Yu. N.⁷,Grenfell John L.⁸,Rauer Heike⁸,Odert Petra⁹,Leitzinger Martin⁹,Selsis F.¹⁰¹¹,Khodachenko Maxim L.¹²,Eiroa Carlos¹³,Kasting Jim¹⁴,Lammer Helmut¹⁰

Affiliation:

1. Department of Astronomy, University of Texas at Austin, Austin, Texas.

2. Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts.

3. California Institute of Technology/Jet Propulsion Laboratory, Pasadena, California.

4. European Space Agency, ESTEC, Noordwijk, The Netherlands.

5. Institut d'Estudis Espacials de Catalunya, Barcelona, Spain.

6. Instituto de Ciencias del Espacio, Barcelona, Spain.

7. Polar Geophysical Institute, Russian Academy of Sciences, Murmansk, Russian Federation.

8. Institute für Planetenforschung, Extrasolare Planeten und Atmospharen, Berlin, Germany.

9. Institute for Physics, University of Graz;, Graz, Austria.

10. Centre de Recherche en Astrophysique de Lyon; France.

11. École Normale Supérieure, Lyon, France.

12. Space Research Institute, Austrian Academy of Sciences, Graz, Austria.

13. Departemento de Física Teórica, C-XI, Facultad de Ciencias, Universidad Autónoma de Madrid, Madrid, Spain.

14. Department of Geosciences, Pennsylvania State University, State College, Pennsylvania.

Publisher

Mary Ann Liebert Inc

Subject

Space and Planetary Science,Agricultural and Biological Sciences (miscellaneous)

Link

http://www.liebertpub.com/doi/pdf/10.1089/ast.2006.0125

Reference369 articles.

1. Photoevaporation of Circumstellar Disks Due to External Far‐Ultraviolet Radiation in Stellar Aggregates

2. A limit on the presence of Earth-mass planets around a Sun-like star

3. On detecting terrestrial planets with timing of giant planet transits

4. Accretion Efficiency during Planetary Collisions

5. Impact Erosion of Terrestrial Planetary Atmospheres

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