WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY
Van Eylen, V., Lund, M. N., Aguirre, V. Silva, Arentoft, T., Kjeldsen, H., Albrecht, S., Chaplin, W. J., Isaacson, H., Pedersen, M. G., Jessen-Hansen, J., Tingley, B., Christensen-Dalsgaard, J., AertsVolume:
782
Language:
english
Journal:
The Astrophysical Journal
DOI:
10.1088/0004-637X/782/1/14
Date:
February, 2014
File:
PDF, 812 KB
english, 2014