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Analysis of the variability of the luminous emission line star MWC 314

G. Muratorio, C. Rossi, M. Friedjung

Astronomy and Astrophysics · 2008 · 11 citations · 9 references

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Concepts

Abstract

Context. We investigated the surroundings of MWC 314 in the framework of the study of hot emission line star environments using the SAC method. This star is either a B[e] supergiant or a luminous blue variable and appears to be extremely luminous and massive.

References

9

Atomic data from the IRON Project. XIX. Radiative transition probabilities for forbidden lines inFe II

P. Quinet, M. Le Dourneuf, C. J. Zeippen · Astronomy and Astrophysics Supplement Series · 1996 · 102 citations · Full text

, , +13

Kinematical structure of the circumstellar environments of galactic B[e]-type stars

Astronomy and Astrophysics · 2003 · 65 citations · Full text

, , +10

Extended shells around B[e] stars

A. P. Marston, B. McCollum · Astronomy and Astrophysics · 2007 · 57 citations · Full text

, , +17

Stars with the B[e] Phenomenon

M. Kraus, А. С. Мирошниченко · ASPC · 2006 · 46 citations

, , +10

The Origin of Fe<scp>ii</scp>and [Fe<scp>ii</scp>] Emission Lines in the 4000–10000 A Range in the BD Weigelt Blobs of η Carinae

E. M. Verner, T. R. Gull, F. C. Bruhweiler et al. · The Astrophysical Journal · 2002 · 45 citations · Full text

, , +10