Results 61 to 70 of about 114 (114)
It is unclear how directly imaged substellar companions with masses near the deuterium burning limit form, because these objects are rare and their bulk properties are not diagnostic of their formation.
William O. Balmer +17 more
doaj +1 more source
Close-in substellar companions experience strong tidal and magnetic interactions with their host stars and are therefore subject to fast orbital evolution.
Breton S. N. +18 more
doaj +1 more source
Recent observations have confirmed circumplanetary disks (CPDs) embedded in parental protoplanetary disks (PPDs). On the other hand, planetary-mass companions and planetary-mass objects (PMOs) are likely to harbor their own accretion disks.
Xilei Sun +3 more
doaj +1 more source
Molecular Distributions and Abundances in the Binary-shaped Outflow of V Hya
Binaries are known to play a key role in the mass loss and dynamical environments of evolved stars. Stellar and substellar companion interactions produce complex wind morphologies including rotating/expanding disks, bipolar outflows, and spiral wind ...
Mark A. Siebert +3 more
doaj +1 more source
A SURVEY FOR NEW STARS AND BROWN DWARFS IN THE OPHIUCHUS STAR-FORMING COMPLEX. [PDF]
Esplin TL, Luhman KL.
europepmc +1 more source
REFINING THE CENSUS OF THE UPPER SCORPIUS ASSOCIATION WITH <i>GAIA</i>. [PDF]
Luhman KL, Esplin TL.
europepmc +1 more source
A SURVEY FOR NEW MEMBERS OF TAURUS FROM STELLAR TO PLANETARY MASSES. [PDF]
Esplin TL, Luhman KL.
europepmc +1 more source
NEW YOUNG STARS AND BROWN DWARFS IN THE UPPER SCORPIUS ASSOCIATION. [PDF]
Luhman KL +4 more
europepmc +1 more source
SEEDS - Strategic explorations of exoplanets and disks with the Subaru Telescope. [PDF]
Tamura M.
europepmc +1 more source
Post-main-sequence planetary system evolution. [PDF]
Veras D.
europepmc +1 more source

