η Carinae: the Near-Infrared Light-Curves

Details η Carinae: the Near-Infrared Light-Curves η Carinae: the Near-Infrared Light-Curves

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..332..115w&link_type=abstract

The Fate of the Most Massive Stars, ASP Conference Series, Vol. 332, Proceedings of the conference held 23-28 May, 2004 in Grand

Astronomy and Astrophysics

Astronomy

Scientific paper

Photometric monitoring of η Car over the last 32 years shows secular, periodic and quasi-periodic variations at near-infrared wavelengths. Most of the flux at JHKL is free-free emission from the central star and its immediate surrounds; only at L is there a possible contribution from hot dust. The L-band and X-ray flux show a remarkable degree of similarity in the morphology of their light curves at the time of the spectroscopic events.

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