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Monday, July 1 - Session 1 - 14:00 |
![]() C. Catala
Observatoire de Paris, LESIA, 5 place Jules Janssen 92195 Meudon, France
Intermediate mass pre-main sequence stars (between 1.5 and 5 solar
masses) cross the instability strip on their way toward the main sequence.
They are therefore expected to be pulsating in a similar way as the
Last changed: 2002/Jun/04
©1996-2002 CAUP |