We present extensive spectroscopic and photometric monitoring of two famous and currently highly active luminous blue variables (LBVs) in the Large Magellanic Cloud (LMC), together with more limited coverage of three further, lesser known members of the class. R127 was discovered as an Ofpe/WN9 star in the 1970s but entered a classical LBV outburst in or about 1980 that is still in progress, thus enlightening us about the minimum state of such objects. R71 is currently the most luminous star in the LMC and continues to provide surprises, such as the appearance of [Ca ii] emission lines, as its spectral type becomes unprecedentedly late. Most recently, R71 has developed inverse P Cyg profiles in many metal lines. The other objects are as fol...
Motivated by the detection of a recent outburst of the massive luminous blue variable LMC-R71, which...
We have discovered that R143 in the Large Magellanic Cloud is a luminous blue variable (LBV), the fi...
Context. Previous studies have concluded that low- and intermediate-mass stars cannot account for th...
We present extensive spectroscopic and photometric monitoring of two famous and currently highly act...
The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the in...
Context. Luminous blue variables (LBVs) are evolved massive stars that exhibit instabilities that ar...
We performed a spectroscopic and photometric analysis to study new eruptions in two luminous blue va...
Luminous Blue Variable stars (LBVs) are evolved massive stars that undergo instabilities and experie...
Motivated by the detection of a recent outburst of the massive luminous blue variable LMC-R71, which...
The nebulae associated with four luminous blue variables (LBVs) in the Large Magellanic Cloud (LMC) ...
CONTEXT: The RAVE spectroscopic survey for galactic structure and evolution obtains 8400-8800 Ang sp...
Context. The RAVE spectroscopic survey for galactic structure and evolution obtains 8400–8800 Å sp...
We have discovered that R143 in the Large Magellanic Cloud is a luminous blue variable (LBV), the fi...
Motivated by the detection of a recent outburst of the massive luminous blue variable LMC-R71, which...
We have discovered that R143 in the Large Magellanic Cloud is a luminous blue variable (LBV), the fi...
Context. Previous studies have concluded that low- and intermediate-mass stars cannot account for th...
We present extensive spectroscopic and photometric monitoring of two famous and currently highly act...
The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the in...
Context. Luminous blue variables (LBVs) are evolved massive stars that exhibit instabilities that ar...
We performed a spectroscopic and photometric analysis to study new eruptions in two luminous blue va...
Luminous Blue Variable stars (LBVs) are evolved massive stars that undergo instabilities and experie...
Motivated by the detection of a recent outburst of the massive luminous blue variable LMC-R71, which...
The nebulae associated with four luminous blue variables (LBVs) in the Large Magellanic Cloud (LMC) ...
CONTEXT: The RAVE spectroscopic survey for galactic structure and evolution obtains 8400-8800 Ang sp...
Context. The RAVE spectroscopic survey for galactic structure and evolution obtains 8400–8800 Å sp...
We have discovered that R143 in the Large Magellanic Cloud is a luminous blue variable (LBV), the fi...
Motivated by the detection of a recent outburst of the massive luminous blue variable LMC-R71, which...
We have discovered that R143 in the Large Magellanic Cloud is a luminous blue variable (LBV), the fi...
Context. Previous studies have concluded that low- and intermediate-mass stars cannot account for th...