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The “Living with a Red Dwarf” program: XUV radiation and plasma environments of hosted planets and impacts on habitability

Published online by Cambridge University Press:  21 October 2010

Edward F. Guinan
Affiliation:
Department of Astronomy & Astrophysics, Villanova University, 800 E. Lancaster Ave, Villanova, PA 19085USA email: [email protected]
Scott G. Engle
Affiliation:
Department of Astronomy & Astrophysics, Villanova University, 800 E. Lancaster Ave, Villanova, PA 19085USA email: [email protected]
Trisha Mizusawa
Affiliation:
Department of Astronomy & Astrophysics, Villanova University, 800 E. Lancaster Ave, Villanova, PA 19085USA email: [email protected]
George P. McCook
Affiliation:
Department of Astronomy & Astrophysics, Villanova University, 800 E. Lancaster Ave, Villanova, PA 19085USA email: [email protected]
A. Wolfe
Affiliation:
Department of Astronomy & Astrophysics, Villanova University, 800 E. Lancaster Ave, Villanova, PA 19085USA email: [email protected]
Jeffrey Coughlin
Affiliation:
Department of Astronomy & Astrophysics, Villanova University, 800 E. Lancaster Ave, Villanova, PA 19085USA email: [email protected]
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Abstract

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We describe the LWARD program on dM stars and habitability in their environment.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Guinan, E. F & Engle, S. G. 2009, arXiv:0901.1860Google Scholar
Guinan, E. F., Engle, S. G., & Dewarf, L. E. 2009, in: Future Directions in Ultraviolet Spectroscopy, American Institute of Physics Conf. Proc., Vol. 1135, p. 244Google Scholar