Dust Obscuration events of the Symbiotic Nova RR Tel in the near IR

Details Dust Obscuration events of the Symbiotic Nova RR Tel in the near IR Dust Obscuration events of the Symbiotic Nova RR Tel in the near IR

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20..225k&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

Binaries: Symbiotic, Circumstellar Matter, Novae, Cataclysmic Variables, Stars: Individual (Rr Tel)

Scientific paper

By use of ground based IR photometry, we have studied the dust obscuration events of the symbiotic nova RR Tel which is a binary composed of a cool mira and a hot white dwarf. The JHKL light curves were corrected for Mira pulsations and correlated to the AAVSO visual light curve. We compare the behaviour of the three obscurations in different wavelength bands and propose interpretations of the results.

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