J/other/Ap/54.81     Spectroscopy of θ1 Ori C system  (Vitrichenko+, 2011)

Runaway spectral double star from the theta1 Ori C system. Vitrichenko E.A., Tsymbal V., Bychkova L, Bychkov V. <Astrophysics, 54, 81 (2011)> =2011Ap.....54...81V 2011Ap.....54...81V
ADC_Keywords: Stars, double and multiple; Spectroscopy; Equivalent widths Keywords: stars: runaway stars - stars: binary stars - individual: theta1 Ori C Abstract: The spectral-double system escaping from multiple system theta1 Ori C is investigated. Radial velocities of both components are measured, for them are constructed and solved curves of radial velocity. Physical parameters of stars and their chemical composition are determined. Description: High quality spectra of the triple star theta1 Ori C in the Orion Trapezium show that one more star in this system is a spectral binary. Its components are young main-sequence A-stars with masses of 1.3 and 1.4 solar mass. Radial velocities of stellar lines indicate that this binary runs away from the system in the direction to an observer with a large negative velocity. For the primary star (C3p) and the secondary (C3s) a list of lines, wavelength and equivalent width are given. Objects: ----------------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------------- 05 35 16.5 -05 23 23 tet01 Ori C = HD 37022 ----------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table.dat 28 376 Equivalent widths of lines for the θ1 Ori C3 stars -------------------------------------------------------------------------------- Byte-by-byte Description of file: table.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 A3 --- Ion Name of ion 6- 12 F7.2 0.1nm lambda [4600/6600] Wavelength in Angstroms 15- 20 F6.4 0.1nm EWC3p ? Equivalent width for C3p component 23- 28 F6.4 0.1nm EWC3s ? Equivalent width for C3s component -------------------------------------------------------------------------------- Acknowledgements: Nataly Bondar', otbn(at)mail.ru
(End) Eduard Vitrichenko [SRI, Russia], Patricia Vannier [CDS] 17-Mar-2011
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