MWC 930 — a new luminous blue variable candidate

We present the results of optical high-resolution and near-infrared low-resolution spectroscopy and multicolour optical and near-infrared photometry of the emission-line star MWC 930. The spectrum is rich with Fe ii emissions, most of which have P Cyg-type profiles. The emission lines are strong and...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2005-11, Vol.364 (1), p.335-343
Hauptverfasser:	Miroshnichenko, A. S., Bjorkman, K. S., Grosso, M., Levato, H., Grankin, K. N., Rudy, R. J., Lynch, D. K., Mazuk, S., Puetter, R. C.
Format:	Artikel
Sprache:	eng
Schlagworte:	circumstellar matter Luminosity Spectrum analysis stars: emission-line stars: emission‐line, Be stars: individual: MWC 930 techniques: photometric techniques: spectroscopic Velocity
Online-Zugang:	Volltext
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