Multiplicity Study of exoplanet host stars: The HD3651AB system
M. Mugrauer, A. Seifahrt, R. Neuhaeuser, T. Mazeh, T. Schmidt
Abstract
We report on new results of our multiplicity study and present our follow-up observations of the recently detected faint companion HD3651B, the first directly imaged T dwarf companion of an exoplanet host star.
Create a lesson
Related papers
On binary pulsars and the force of gravity
Davor Palle
Tidal torques. A critical review of some techniques
Michael Efroimsky, James G. Williams
Dynamics of a Spherical Accretion Shock with Neutrino Heating and Alpha-Particle Recombination
Rodrigo Fernández, Christopher Thompson
Asymptotically FRW black holes
J. T. Firouzjaee, Reza Mansouri
Reaction of Accretion Disks to Abrupt Mass Loss During Binary Black Hole Merger
Sean M. O'Neill, M. Coleman Miller, Tamara Bogdanovic et al.
A Gamma-Ray Burst/Pulsar for Cosmic-Ray Positrons with a Dark Matter-like Spectrum
Kunihito Ioka