The binary nature of the central star of the planetary nebula LT-5

Details The binary nature of the central star of the planetary nebula LT-5 The binary nature of the central star of the planetary nebula LT-5

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127l...5s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 1, Oct. 1983, p. L5, L6.

Astronomy and Astrophysics

Astrophysics

17

Binary Stars, Light Curve, Planetary Nebulae, Ubv Spectra, Electrophotometry, Hot Stars, Stellar Spectrophotometry

Scientific paper

Photoelectric photometry of the central star of the planetary nebula is
presented, including both UBV observations and light curves. The results
show periodic variations of small amplitude in U, B, and V. It is
suggested that this variation is probably caused by the reflection
effect in a binary system.

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