Two new LBV stars have been discovered in the Andromeda Galaxy. Since the
middle of the last century, only four such objects had been known in this
galaxy, they were discovered by American scientists Edwin Hubble and Allan
Sandage with colleagues. Astronomers from SAO added two more stars to this
list in 2015. LBV stars (Luminous Blue Variables) are very massive, they are
born with masses greater than 50 solar masses. These stars are very rare:
for each such a star with a mass of more than 50 solar masses, over 30000
less massive stars are born. Once the hydrogen thermonuclear fuel comes to
the end in the center of very massive stars, the stars strongly change their
brightness, and after a few ten thousand years they blow up as supernovae.
We have found a new method to search for LBV stars, which is based on their
intrinsic property: when such a star decreases in size (the star's
photosphere contracts), its photospheric temperature gets higher, the star's
brightness dims; when the star expands, it cools and becomes brighter. In
Figure 1 the spectral energy distributions for six stars are shown: upper
row - the newly discovered LBV stars, middle row - two well-known LBV stars
Var A-1 and AE And, the lower row - two new B[e]-supergiant stars in
Andromeda. The two classical LBVs and our LBVs do change their brightness
strongly in accordance with our models. The two stars in the lower row do
not change their brightness, but they have strong infrared excesses. The
B[e]-supergiants are probably the same as LBVs, but they may be located in
close binaries. Therefore they cannot change their brightness but have
instead strong disk-like dust envelopes. The optical spectra were obtained
with the BTA telescope, the infrared spectra were taken (simultaneously) in
the USA (the Apache Point Observatory). The infrared spectra are shown in
Figure 2, strong emission lines of hydrogen (Pa and Br series), helium,
iron, and nitrogen are seen in the spectra.
Published:
Sholukhova, O., Bizyaev, D., Fabrika, S., Sarkisyan, A., Malanushenko, V.,
Valeev, A.,
Monthly Notices of the Royal Astronomical Society, 447, 2459-2467, 2015
Contact - S.N.Fabrika
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