@inproceedings{86045ab6dcc1471eabccb8f2402c519e,
title = "On the habitability of terrestrial planets in binary star systems",
abstract = "The growing number of detected planets in binary star systems requires methods for a quick assessment of possible habitability of planets in such environments. We offer an analytic method to determine habitability of a terrestrial planet in binary star systems. In this context we give an answer to the most important question: Do the radiative and gravitational perturbations of a secondary influence the extent of the habitable zone (HZ)? After we have defined the borders of the HZ, we will show the dynamical behaviour of a terrestrial planet in the HZ when adding a Jupiter to the system. In such a system the HZ shows signs of mean motion resonances and secular resonances, depending on the architecture of the planetary system.",
keywords = "Binaries: general, n-body simulations, numerical, planetary systems",
author = "Elke Pilat-Lohinger and Barbara Funk and Siegfried Eggl",
year = "2012",
month = aug,
doi = "10.1017/S1743921313012702",
language = "English (US)",
isbn = "9781107033825",
series = "Proceedings of the International Astronomical Union",
publisher = "Cambridge University Press",
number = "S293",
pages = "140--145",
booktitle = "Formation, Detection, and Characterization of Extrasolar Habitable Planets",
address = "United Kingdom",
edition = "S293",
}