[HTML][HTML] Hard X-ray identification of η Carinae and steadiness close to periastron
JC Leyder - Astronomy & Astrophysics, 2010 - aanda.org
Context. The colliding-wind binary η Carinae exhibits soft X-ray thermal emission that varies
strongly around the periastron passage. It has been found to have non-thermal emission …
strongly around the periastron passage. It has been found to have non-thermal emission …
[PDF][PDF] Hard X-ray identification of η Carinae and steadiness close to periastron
JC Leyder, R Walter, G Rauw - 2018 - researchgate.net
Context. The colliding-wind binary η Carinae exhibits soft X-ray thermal emission that varies
strongly around the periastron passage. It has been found to have non-thermal emission …
strongly around the periastron passage. It has been found to have non-thermal emission …
Hard X-ray identification of η Carinae and steadiness close to periastron
JC Leyder, R Walter, G Rauw - Astronomy and Astrophysics, 2010 - ui.adsabs.harvard.edu
Context. The colliding-wind binary η Carinae exhibits soft X-ray thermal emission that varies
strongly around the periastron passage. It has been found to have non-thermal emission …
strongly around the periastron passage. It has been found to have non-thermal emission …
Hard X-ray identification of η Carinae and steadiness close to periastron
JC Leyder, R Walter, G Rauw - Astronomy and Astrophysics, 2010 - orbi.uliege.be
Context. The colliding-wind binary η Carinae exhibits soft X-ray thermal emission that varies
strongly around the periastron passage. It has been found to have non-thermal emission …
strongly around the periastron passage. It has been found to have non-thermal emission …
[PDF][PDF] Hard X-ray identification of η Carinae and steadiness close to periastron
JC Leyder, R Walter, G Rauw - 2010 - Citeseer
Context. The colliding-wind binary η Carinae exhibits soft X-ray thermal emission that varies
strongly around the periastron passage. It has been found to have non-thermal emission …
strongly around the periastron passage. It has been found to have non-thermal emission …
[PDF][PDF] Hard X-ray identification of η Carinae and steadiness close to periastron
JC Leyder, R Walter, G Rauw - A&A, 2010 - scholar.archive.org
Context. The colliding-wind binary η Carinae exhibits soft X-ray thermal emission that varies
strongly around the periastron passage. It has been found to have non-thermal emission …
strongly around the periastron passage. It has been found to have non-thermal emission …
[引用][C] Hard X-ray identification ofη Carinae and steadiness close to periastron
JC Leyder, R Walter, G Rauw - Astronomy & Astrophysics, 2010 - cir.nii.ac.jp
Hard X-ray identification of<i>η</i> Carinae and steadiness close to periastron | CiNii Research
CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データを …
CiNii 国立情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データを …
Hard X-ray identification of Eta Carinae and steadiness close to periastron
JC Leyder, R Walter, G Rauw - arXiv preprint arXiv:1008.5366, 2010 - arxiv.org
Context: The colliding-wind binary Eta Car exhibits soft X-ray thermal emission that varies
strongly around periastron, and non-thermal emission seen in hard X-rays and gamma-rays …
strongly around periastron, and non-thermal emission seen in hard X-rays and gamma-rays …
[引用][C] Hard X-ray identification of η Carinae and steadiness close to periastron
JC LEYDER, R WALTER… - … and astrophysics (Berlin …, 2010 - pascal-francis.inist.fr
Hard X-ray identification of η Carinae and steadiness close to periastron CNRS Inist Pascal-Francis
CNRS Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …
CNRS Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …
[PDF][PDF] Hard X-ray identification of η Carinae and steadiness close to periastron
JC Leyder, R Walter, G Rauw - A&A, 2010 - scholar.archive.org
Context. The colliding-wind binary η Carinae exhibits soft X-ray thermal emission that varies
strongly around the periastron passage. It has been found to have non-thermal emission …
strongly around the periastron passage. It has been found to have non-thermal emission …