Light Time Effects in Pulsating Variables and Brown Dwarfs

Details Light Time Effects in Pulsating Variables and Brown Dwarfs Light Time Effects in Pulsating Variables and Brown Dwarfs

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003iaus..211..313y&link_type=abstract

Brown Dwarfs, Proceedings of IAU Symposium #211, held 20-24 May 2002 at University of Hawaii, Honolulu, Hawaii. Edited by Eduard

Astronomy and Astrophysics

Astronomy

Scientific paper

Dwarf cepheids DY Her, AD CMi, and BE Lyn show light time effects, which
may be caused by orbital motion due to a low mass unseen companion.
Their mass is probably between 0.015 to 0.07 M&sun;, so they
may be brown dwarfs.

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