luminous blue variable
(LBV, S Doradus variable)
(type of extremely bright variable stars)
A luminous blue variable (LBV or S Doradus variable after
an example in the Large Magellanic Cloud) is a classification
of variable star that is extremely bright and extremely rare.
They are the most luminous stars known, with luminosities
hundreds of thousands times that of the Sun
and some of them experience outbursts (LBV outbursts) bright enough to be
mistaken for supernovae.
They are also among the most massive stars, up to 100 solar masses.
In addition to those found in the Milky Way,
examples have been identified in other galaxies including the
Magellanic Clouds, Andromeda, and Triangulum Galaxy, and they have been
used to estimate distances to the latter two galaxies.
Explanation of their structure and evolution
continues to be a topic of research.
(star type,variable)
Further reading:
https://en.wikipedia.org/wiki/Luminous_blue_variable
http://www.star.ucl.ac.uk/~pac/paper/node8.html
https://ui.adsabs.harvard.edu/abs/2020Galax...8...20W/abstract
https://www.cosmos.esa.int/documents/739790/758039/SP08-KWeis.pdf/e397df29-06bd-4f4b-b093-5585110e1295
https://www.rochesterastronomy.org/snimages/lbvlist.html
https://ui.adsabs.harvard.edu/abs/2020MNRAS.497..687S/abstract
Referenced by pages:
Eta Carinae (η Car)
variable star
Index