N ii λλ5668–5712: A NEW CLASS OF SPECTRAL FEATURES IN ETA CARINAE
A Mehner, K Davidson, GJ Ferland - The Astrophysical Journal, 2011 - iopscience.iop.org
We report on the N ii λλ5668–5712 emission and absorption lines in the spectrum of η
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
[PDF][PDF] N II λλ5668-5712: A New Class of Spectral Features in Eta Carinae
A Mehner, K Davidson, G Ferland - THE ASTROPHYSICAL JOURNAL, 2011 - Citeseer
We report on the N II λλ5668–5712 emission and absorption lines in the spectrum of η
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
N II {lambda}{lambda} 5668-5712: A NEW CLASS OF SPECTRAL FEATURES IN ETA CARINAE
A Mehner, K Davidson, GJ Ferland - Astrophysical Journal, 2011 - osti.gov
We report on the N II {lambda}{lambda} 5668-5712 emission and absorption lines in the
spectrum of {eta} Carinae. Spectral lines of the stellar wind regions can be classified into …
spectrum of {eta} Carinae. Spectral lines of the stellar wind regions can be classified into …
[引用][C] N II λλ5668−5712: A NEW CLASS OF SPECTRAL FEATURES IN ETA CARINAE
A Mehner, K Davidson, GJ Ferland - The Astrophysical Journal, 2011 - cir.nii.ac.jp
N II λλ5668−5712: A NEW CLASS OF SPECTRAL FEATURES IN ETA CARINAE $^,$ | 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 …
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 …
N II λλ5668-5712: A New Class of Spectral Features in Eta Carinae
A Mehner, K Davidson… - The Astrophysical …, 2011 - ui.adsabs.harvard.edu
We report on the N II λλ5668-5712 emission and absorption lines in the spectrum of η
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
N II λλ5668-5712: A NEW CLASS OF SPECTRAL FEATURES IN ETA CARINAE
A Mehner, K Davidson, GJ Ferland - Astrophysical Journal, 2011 - inis.iaea.org
[en] We report on the N II λλ5668-5712 emission and absorption lines in the spectrum of η
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
[引用][C] NII λλ5668-5712: A NEW CLASS OF SPECTRAL FEATURES IN ETA CARINAE*,† t
A MEHNER, K DAVIDSON… - The Astrophysical …, 2011 - pascal-francis.inist.fr
NII λλ5668-5712: A NEW CLASS OF SPECTRAL FEATURES IN ETA CARINAE*,†t CNRS Inist
Pascal-Francis CNRS Pascal and Francis Bibliographic Databases Simple search Advanced …
Pascal-Francis CNRS Pascal and Francis Bibliographic Databases Simple search Advanced …
N II λλ5668-5712: A New class of spectral features in eta Carinae
A Mehner, K Davidson, GJ Ferland - Astrophysical Journal, 2011 - experts.umn.edu
We report on the N II λλ5668-5712 emission and absorption lines in the spectrum of η
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
[PDF][PDF] N II λλ5668− 5712: A New Class of Spectral Features in Eta Carinae
A Mehner, K Davidson, GJ Ferland - 2011 - core.ac.uk
We report on the N II λλ5668–5712 emission and absorption lines in the spectrum of η
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
[PDF][PDF] N II λλ5668− 5712: A New Class of Spectral Features in Eta N II 5668− 5712: A New Class of Spectral Features in Eta Carinae
A Mehner, K Davidson, GJ Ferland - 2011 - uknowledge.uky.edu
We report on the N II λλ5668–5712 emission and absorption lines in the spectrum of η
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …
Carinae. Spectral lines of the stellar wind regions can be classified into four physically …