The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the intermediate, peculiar early-B state, and substantially fainter in visual light, signaling the final decline from its major outburst that began between 1978 and 1980. This transformation was detected in 2008 January, but archival data show that it began between early 2005 and early 2007. In fact, significant changes from the maximum, peculiar A-type spectrum, which was maintained from 1986 through 1998, had already begun the following year, coinciding with a steep drop in visual light. We show detailed correspondences between the spectrum and light, in which the decline mimics the rise. Moreover, these trends are not monotonic but are ...
Massive stars play a significant role in the shaping and evolution of the Galaxy. Their stellar wind...
We report the first results of a long term infrared monitoring campaign of known and candidate galac...
We present observations of the massive transitional star W243 in Westerlund 1 . We find an apparent ...
The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the in...
We present extensive spectroscopic and photometric monitoring of two famous and currently highly act...
Context. Luminous blue variables (LBVs) are evolved massive stars that exhibit instabilities that ar...
Context. The RAVE spectroscopic survey for galactic structure and evolution obtains 8400–8800 Å sp...
CONTEXT: The RAVE spectroscopic survey for galactic structure and evolution obtains 8400-8800 Ang sp...
Context. Luminous blue variables (LBVs) are a class of highly unstable stars that have been proposed...
Context. Luminous blue variables (LBVs) are a class of highly unstable stars that have been proposed...
Motivated by the detection of a recent outburst of the massive luminous blue variable LMC-R71, which...
Aims. The luminous blue variable (LBV) R71 is currently undergoing an eruption, which differs photom...
Aims. So far the highly unstable phase of luminous blue variables (LBVs) has not been understood wel...
Context. Luminous blue variables (LBVs) are a class of highly unstable stars that have been proposed...
Massive stars play a significant role in the shaping and evolution of the Galaxy. Their stellar wind...
We report the first results of a long term infrared monitoring campaign of known and candidate galac...
We present observations of the massive transitional star W243 in Westerlund 1 . We find an apparent ...
The paradigmatic luminous blue variable R127 in the Large Magellanic Cloud has been found in the in...
We present extensive spectroscopic and photometric monitoring of two famous and currently highly act...
Context. Luminous blue variables (LBVs) are evolved massive stars that exhibit instabilities that ar...
Context. The RAVE spectroscopic survey for galactic structure and evolution obtains 8400–8800 Å sp...
CONTEXT: The RAVE spectroscopic survey for galactic structure and evolution obtains 8400-8800 Ang sp...
Context. Luminous blue variables (LBVs) are a class of highly unstable stars that have been proposed...
Context. Luminous blue variables (LBVs) are a class of highly unstable stars that have been proposed...
Motivated by the detection of a recent outburst of the massive luminous blue variable LMC-R71, which...
Aims. The luminous blue variable (LBV) R71 is currently undergoing an eruption, which differs photom...
Aims. So far the highly unstable phase of luminous blue variables (LBVs) has not been understood wel...
Context. Luminous blue variables (LBVs) are a class of highly unstable stars that have been proposed...
Massive stars play a significant role in the shaping and evolution of the Galaxy. Their stellar wind...
We report the first results of a long term infrared monitoring campaign of known and candidate galac...
We present observations of the massive transitional star W243 in Westerlund 1 . We find an apparent ...