The traditional theory of stellar structure and evolution, presuming that stars formed and evolved in isolation, and the effect of rotation is negligible, is now a view of the past. Recent studies bas...
Meteorites display an isotopic composition dichotomy between non-carbonaceous (NC) and carbonaceous (CC) groups, indicating that planetesimal formation in the solar protoplanetary disk occurred in two...
To date, more than 3000 exoplanetary systems have been observed. Different kinds of planetary configurations are reported. Such as near-resonant configuration, closely packed multiple planetary system...
Magnetic fields play an important role in the evolution of interstellar medium and star formation. As the only direct tracer of interstellar field strength, credible Zeeman measurements remain sparse ...
In this talk the speaker will review their current understanding of giant planet and binary star formation, highlighting the key similarities and unique unknowns for each process. She will show how cu...