Model of molecular non-LTE emission in exoplanetary atmospheres

Details Model of molecular non-LTE emission in exoplanetary atmospheres Model of molecular non-LTE emission in exoplanetary atmospheres

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..363d&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.363

Physics

Scientific paper

The observations by transit spectroscopy of exoplanetary atmospheres give the first insight into the atmospheric physics of these objects [1,2] Observations of anomalous emission in the near infrared have challenged interpretation of exoplanetary spectra [1]. A model of non-LTE emission is presented to support the interpretation of K and L band excess emission.

Affiliated with

Also associated with

No associations

Rating

Model of molecular non-LTE emission in exoplanetary atmospheres does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Model of molecular non-LTE emission in exoplanetary atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Model of molecular non-LTE emission in exoplanetary atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1477102