Explaining the early exit of Eta Carinae from its 2009 X-ray minimum with the accretion model
We use the accretion model to explain the early exit of η Car from its 2009 X-ray minimum. In
the accretion model, the secondary star accretes mass from the primary wind near periastron …
the accretion model, the secondary star accretes mass from the primary wind near periastron …
EXPLAINING THE EARLY EXIT OF ETA CARINAE FROM ITS 2009 X-RAY MINIMUM WITH THE ACCRETION MODEL
A Kashi, N Soker - Astrophysical Journal (Online), 2009 - osti.gov
We use the accretion model to explain the early exit of {eta} Car from its 2009 X-ray
minimum. In the accretion model, the secondary star accretes mass from the primary wind …
minimum. In the accretion model, the secondary star accretes mass from the primary wind …
[PDF][PDF] EXPLAINING THE EARLY EXIT OF ETA CARINAE FROM ITS 2009 X-RAY MINIMUM WITH THE ACCRETION MODEL
A KASHI, N SOkER - THE ASTROPHYSICAL JOURNAL, 2009 - scholar.archive.org
We use the accretion model to explain the early exit of η Car from its 2009 X-ray minimum. In
the accretion model, the secondary star accretes mass from the primary wind near periastron …
the accretion model, the secondary star accretes mass from the primary wind near periastron …
Explaining the Early Exit of Eta Carinae from its 2009 X-Ray Minimum with the Accretion Model
A Kashi, N Soker - The Astrophysical Journal, 2009 - ui.adsabs.harvard.edu
We use the accretion model to explain the early exit of η Car from its 2009 X-ray minimum. In
the accretion model, the secondary star accretes mass from the primary wind near periastron …
the accretion model, the secondary star accretes mass from the primary wind near periastron …
[PDF][PDF] EXPLAINING THE EARLY EXIT OF ETA CARINAE FROM ITS 2009 X-RAY MINIMUM WITH THE ACCRETION MODEL
A Kashi, N Soker - arXiv preprint arXiv:0904.2840, 2009 - Citeseer
We use the accretion model to explain the early exit of η Car from its 2009 X-ray minimum. In
the accretion model the secondary star accretes mass from the primary wind near periastron …
the accretion model the secondary star accretes mass from the primary wind near periastron …
Explaining the Early Exit of Eta Carinae from its 2009 X-Ray Minimum with the Accretion Model
A Kashi, N Soker - arXiv preprint arXiv:0904.2840, 2009 - arxiv.org
We use the accretion model to explain the early exit of Eta Carinae from its 2009 X-ray
minimum. In the accretion model the secondary star accretes mass from the primary wind …
minimum. In the accretion model the secondary star accretes mass from the primary wind …
[PDF][PDF] EXPLAINING THE EARLY EXIT OF ETA CARINAE FROM ITS 2009 X-RAY MINIMUM WITH THE ACCRETION MODEL
A Kashi, N Soker - arXiv preprint arXiv:0904.2840, 2009 - researchgate.net
We use the accretion model to explain the early exit of η Car from its 2009 X-ray minimum. In
the accretion model the secondary star accretes mass from the primary wind near periastron …
the accretion model the secondary star accretes mass from the primary wind near periastron …
[引用][C] EXPLAINING THE EARLY EXIT OF ETA CARINAE FROM ITS 2009 X-RAY MINIMUM WITH THE ACCRETION MODEL
A Kashi, N Soker - The Astrophysical Journal, 2009 - cir.nii.ac.jp
EXPLAINING THE EARLY EXIT OF ETA CARINAE FROM ITS 2009 X-RAY MINIMUM WITH
THE ACCRETION MODEL | CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ …
THE ACCRETION MODEL | CiNii Research CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ …
EXPLAINING THE EARLY EXIT OF ETA CARINAE FROM ITS 2009 X-RAY MINIMUM WITH THE ACCRETION MODEL
A Kashi, N Soker - Astrophysical Journal (Online), 2009 - inis.iaea.org
[en] We use the accretion model to explain the early exit of η Car from its 2009 X-ray
minimum. In the accretion model, the secondary star accretes mass from the primary wind …
minimum. In the accretion model, the secondary star accretes mass from the primary wind …
Explaining the early exit of ETA carinae from its 2009 X-ray minimum with the accretion model
A Kashi, N Soker - Astrophysical Journal, 2009 - experts.umn.edu
We use the accretion model to explain the early exit of η Car from its 2009 X-ray minimum. In
the accretion model, the secondary star accretes mass from the primary wind near periastron …
the accretion model, the secondary star accretes mass from the primary wind near periastron …