Previous abstract Next abstract
Session 26 - Proto Stars to Supernovae.
Oral session, Monday, June 08
Recent observations of the X-ray emission from the very luminous star Eta Carinae by RXTE, ASCA, and SAX prove that the X-ray variability first reported by ROSAT in 1992 (Corcoran et al. 1995) is periodic. The X-ray lightcurve undergoes a "low state" every 5.5 years which appears to be an occultation event. The X-ray low state coincides with the disappearance of excited He lines which mark the recurrence of the so-called "shell events" (Damineli 1996). We discuss the behavior of the X-ray emission during the most recent "low state" and consider observed variations in column density and observed and intrinsic source brightness in terms of binary and single-star models.
The author(s) of this abstract have provided an email address for comments about the abstract: firstname.lastname@example.org
Program listing for Monday