Will HR8752 become a P Cygni type star?
As long as the yellow hypergiant HR8752 has been observed spectroscopically it has shown erratic and significant fluctuations in its effective temperature. But an impressive and hitherto never observed rise in its temperature started around 1985. Since that time Teff has risen from 4600 K to 7900 K. Regular further observations are needed to see if
de Jager, C. et al.
Fecha de publicación:
6
2001