Periodic Spectral Variations of THETA-1-ORIONIS-C

Details Periodic Spectral Variations of THETA-1-ORIONIS-C Periodic Spectral Variations of THETA-1-ORIONIS-C

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...274l..29s&link_type=abstract

Astronomy and Astrophysics, Vol. 274, NO. 1/JUL(I), P. L29, 1993

Astronomy and Astrophysics

Astrophysics

45

Θl Orionis C, Stars: Early-Type, Emission-Line, Variable

Scientific paper

We have detected periodic spectral variations with a period of 15.43
± 0.03 days in the spectrum of θl Ori C, the
brightest star in the Orion Trapezium and the main source of ionization
of the Orion nebula (M 42).

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