J.C. Martin (U. Illinois-Springfield) et al recently noted
in IAU Circular 8961 the appearance of broad He II emission
lines in the spectrum of the luminous blue variable Eta Carinae.
Such spectral changes are an early precursor of the cyclical
spectroscopic events that occur in eta Carinae every 5.5 years,
and are expected to occur again in early 2009. Increased
observational coverage of eta Car -- including both visual
estimates and high-precision photometry -- are encouraged
beginning now and continuing through 2009 at least. We note
that this star is currently a part of the AAVSO Photoelectric
Photometry program; please use SAO 238242 (V = 5.075) as the
comparison star and SAO 238483 (V = 6.470) as the check star
if you are using the PEPObs data submission tool in Blue & Gold.
Please submit data to the AAVSO as "ETA CAR" (AUID 000-BBR-655).
Charts for Eta Carinae may be generated with VSP:
http://www.aavso.org/observing/charts/vsp/index.html?pickname=eta%20car
This AAVSO Special Notice was prepared by Matthew Templeton.
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