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BCD spectrophotometry for massive stars in transition phases
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Reddening-Free Q Parameters to Classify B-Type Stars with Emission Lines
Gaia EDR3 Confirms that Westerlund 1 is Closer and Older than Previously Thought
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The Blue Supergiant Progenitor of the Supernova Imposter AT 2019krl
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Modeling the remnants of core-collapse supernovae from luminous blue variable stars
A Kostenkov, S Fabrika, O Sholukhova, A Sarkisyan and D Bizyaev Monthly Notices of the Royal Astronomical Society 496(4) 5455 (2020) https://doi.org/10.1093/mnras/staa1824
A New Candidate Luminous Blue Variable
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Wray 15-906: a candidate luminous blue variable discovered with WISE, Herschel, and SALT
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Near-infrared Characterization of Four Massive Stars in Transition Phases*
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Candidate LBV stars in galaxy NGC 7793 found via HST photometry + MUSE spectroscopy
Aida Wofford, Vanesa Ramírez, Janice C Lee, et al. Monthly Notices of the Royal Astronomical Society 493(2) 2410 (2020) https://doi.org/10.1093/mnras/staa290
The History Goes On: Century Long Study of Romano’s Star
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Jose H Groh, Keivan G Stassun, Maria R Drout, et al. Monthly Notices of the Royal Astronomical Society 488(2) 1760 (2019) https://doi.org/10.1093/mnras/stz1712
A slowly expanding torus associated with the candidate LBV MGE 042.0787+00.5084
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New luminous blue variable candidates in NGC 4736
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Catching a star before explosion: the luminous blue variable progenitor of SN 2015bh
Optical spectroscopy of the blue supergiant Sk−69° 279 and its circumstellar shell with SALT
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Extended VHEγ-ray emission towards SGR1806−20, LBV 1806−20, and stellar cluster Cl* 1806−20
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O. V. Maryeva, E. L. Chentsov, V. P. Goranskij, et al. Monthly Notices of the Royal Astronomical Society 458(1) 491 (2016) https://doi.org/10.1093/mnras/stw385
e-MERLIN 21 cm constraints on the mass-loss rates of OB stars in Cyg OB2
J. C. Morford, D. M. Fenech, R. K. Prinja, R. Blomme and J. A. Yates Monthly Notices of the Royal Astronomical Society 463(1) 763 (2016) https://doi.org/10.1093/mnras/stw1914
High-resolution Very Large Array observations of 18 MIPSGAL bubbles
A. Ingallinera, C. Trigilio, P. Leto, et al. Monthly Notices of the Royal Astronomical Society 463(1) 723 (2016) https://doi.org/10.1093/mnras/stw2053
WS1: one more new Galactic bona fide luminous blue variable
A. Y. Kniazev, V. V. Gvaramadze and L. N. Berdnikov Monthly Notices of the Royal Astronomical Society: Letters 449(1) L60 (2015) https://doi.org/10.1093/mnrasl/slv023
Discovery of a new bona fide luminous blue variable in Norma
V. V. Gvaramadze, A. Y. Kniazev and L. N. Berdnikov Monthly Notices of the Royal Astronomical Society 454(4) 3710 (2015) https://doi.org/10.1093/mnras/stv2278
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UKIRT Widefield Infrared Survey for Fe+
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Mass Loss: Its Effect on the Evolution and Fate of High-Mass Stars
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The candidate luminous blue variable G79.29+0.46: a comprehensive study of its ejecta through a multiwavelength analysis
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Confirmation of the Luminous Blue Variable Status of MWC 930
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Search for Southern Galactic Be Star Candidates
B. E. Sabogal, A. García-Varela and R. E. Mennickent Publications of the Astronomical Society of the Pacific 126(937) 219 (2014) https://doi.org/10.1086/675972
One of the most massive stars in the Galaxy may have formed in isolation
L. M. Oskinova, M. Steinke, W.-R. Hamann, et al. Monthly Notices of the Royal Astronomical Society 436(4) 3357 (2013) https://doi.org/10.1093/mnras/stt1817
Fundamental properties of core-collapse supernova and GRB progenitors: predicting the look of massive stars before death
New Galactic Candidate Luminous Blue Variables and Wolf-Rayet Stars
Guy S. Stringfellow, Vasilii V. Gvaramadze, Yuri Beletsky and Alexei Y. Kniazev Proceedings of the International Astronomical Union 7(S282) 267 (2011) https://doi.org/10.1017/S1743921311027542
Spectral variability of LBV star V 532 (Romano’s star)