The orbital kinematics of eta Carinae over three periastra with a possible detection of the elusive secondary's motion [SSA]
arXiver,
http://arxiv.org/abs/2301.00064 The binary eta Carinae is the closest example of a very massive star…
The orbital kinematics of η Carinae over three periastra with a possible detection of the elusive secondary’s motion
Overview of attention for article published in Monthly Notices of the Royal Astronomical Society, January 2023
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