Sub-brown dwarfs as seats of life based on non-polar solvents: Thermodynamic restrictions-Reference-Cited by-同舟云学术

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Sub-brown dwarfs as seats of life based on non-polar solvents: Thermodynamic restrictions

Published:2010-10 Issue:12 Volume:58 Page:1650-1659
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Badescu Viorel

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

1. Physical Chemistry II;Albu,2004

2. Tables of Rosseland mean opacities for candidate atmospheres of life hosting free-floating planets;Badescu;Central European Journal of Physics,2010

3. The Limits of Organic Life in Planetary Systems;Baross,2007

4. Many chemistries could be used to build living systems;Bains;Astrobiology,2004

5. Structural modeling of fluid ethane with Monte Carlo methods;Bassen;Physical Chemistry Chemical Physics,1999

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1. Diving into Exoplanets: Are Water Seas the Most Common?;Astrobiology;2019-05

2. Free-floating planets as potential seats for aqueous and non-aqueous life;Icarus;2011-12

3. Titan under a red dwarf star and as a rogue planet: requirements for liquid methane;Planetary and Space Science;2011-07

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