Analysis of the variability of the luminous emission line star MWC 314-Reference-Cited by-同舟云学术

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

Published:2008-07-01 Issue:2 Volume:487 Page:637-644
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Muratorio G.,Rossi C.,Friedjung M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20078940/pdf

Reference22 articles.

1. Baratta, G. B., Friedjung, M., Muratorio, G., Rossi, C., & Viotti, R. 1998, The Self Absorption Curve Method, A Users` Munual, IAS Internal Report, December 1998

2. Glatzel, W., & Chernigovski, S. 2001, in P Cygni 2000; 400 Years of Progress, ASP Conf. Ser., 233

3. The region of Fe II emission line formation of the symbiotic nova RR Telescopii

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1. BRITE-Constellation reveals evidence for pulsations in the enigmatic binary η Carinae;Monthly Notices of the Royal Astronomical Society;2018-01-18

2. Spectroscopic survey of emission-line stars – I. B[e] stars;Monthly Notices of the Royal Astronomical Society;2015-12-23

3. Spectroscopy,MOSTphotometry, and interferometry of MWC 314: is it an LBV or an interacting binary?;Monthly Notices of the Royal Astronomical Society;2015-11-02

4. MWC 314: binary results from optical interferometry compared with spectroscopy and photometry;SPIE Proceedings;2014-07-24

5. A K-band spectral mini-survey of Galactic B[e] stars★;Monthly Notices of the Royal Astronomical Society;2014-07-17

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