ORBITAL PARAMETERS FOR THE 250M⊙ETA CARINAE BINARY SYSTEM
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/825/i=2/a=105/pdf
Reference83 articles.
1. Wind-wind collision in the Carinae binary system - III. The He II 4686 line profile
2. η CARINAE BABY HOMUNCULUS UNCOVERED BY ALMA
3. Millimeter-wave emission during the 2003 low excitation phase ofηCarinae
4. Accretion of dense clumps in the periastron passage of η Carinae
5. Accretion onto the Companion of η Carinae during the Spectroscopic Event. II. X‐Ray Emission Cycle
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1. Catching the Butterfly and the Homunculus of η Carinae with ALMA;The Astrophysical Journal;2022-08-01
2. The X-Ray Properties of Eta Carinae During Its 2020 X-Ray Minimum;The Astrophysical Journal;2021-06-01
3. Simulating the formation of η Carinae’s surrounding nebula through unstable triple evolution and stellar merger-induced eruption;Monthly Notices of the Royal Astronomical Society;2021-03-01
4. Uncovering the orbital dynamics of stars hidden inside their powerful winds: application to η Carinae and RMC 140;Monthly Notices of the Royal Astronomical Society;2020-03-13
5. Periodicity in the light curve of P Cygni–Indication for a binary companion?;New Astronomy;2018-11
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