Mass loss from Eta Carinae
1979 ◽
Vol 83
◽
pp. 47-50
Keyword(s):
This high luminosity (5 × 106 L⊙) star since 1840 is losing mass at the rate of 7.5 × 10−2 M⊙ per year. The large mass loss could be the result of vibrational instabilities produced in the CNO hydrogen burning phase of a very massive (160 M⊙) star. The presence of high excitation lines in the ultraviolet spectrum of Eta Car suggests the idea of a hot zone excited by dissipation of the supersonic turbulent flow.
1979 ◽
Vol 83
◽
pp. 431-445
◽
Keyword(s):
1989 ◽
Vol 131
◽
pp. 463-472
◽
Keyword(s):
2003 ◽
Vol 209
◽
pp. 447-450
Keyword(s):
1993 ◽
Vol 155
◽
pp. 483-483
Keyword(s):
Keyword(s):
1981 ◽
Vol 59
◽
pp. 465-468
Keyword(s):
1975 ◽
Vol 67
◽
pp. 297-298
1985 ◽
Vol 87
◽
pp. 230-243
◽
Keyword(s):