Search for Infrared Emission from an Exoplanet

Details Search for Infrared Emission from an Exoplanet Search for Infrared Emission from an Exoplanet

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...202.3307h&link_type=abstract

American Astronomical Society Meeting 202, #33.07; Bulletin of the American Astronomical Society, Vol. 35, p.747

Astronomy and Astrophysics

Astronomy

Scientific paper

In recent years, interest in extra-solar planets has spawned extensive efforts to characterize as many aspects of these objects as is observationally and theoretically possible. One area of active research is high-resolution spectroscopy of stars having ``planetary" companions. High resolution spectroscopy of the Jovian planets reveal strong emission of H3+, thus a detection of H3+ in an extra solar object might be plausible. We discuss the sensitivity needed to detect a 'standard Jupiter' around an exoplanet and the limits of our observations.

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