Possible planet formation in the young, low-mass, multiple stellar system GG Tau A.
2014
Investigation of the triple stellar system GG Tau A reveals gas fragments within the central cavity between the Keplerian outer ring orbiting the entire system and the stars themselves; gas flow from this outer ring appears capable of sustaining the inner disk surrounding component star GG Tau Aa beyond the accretion lifetime, leaving time for planet formation to occur.
Keywords:
- Correction
- Source
- Cite
- Save
- Machine Reading By IdeaReader
75
References
84
Citations
NaN
KQI