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Documentation:Aims: We present the first orbital solution for the Wolf-Rayet star, WR 35a, that was discovered by a spectroscopic monitoring of faint WN-type stars. Methods: Spectral features of two different components were identified, and thus a method of disentangling the individual spectra of both components was applied. Radial velocities were determined for each component in the binary system. Results: The orbital solution and component properties of the system were derived. We determined that WR 35a is composed of a WN6 star with a O8.5 V companion orbiting at a 41.90-day period. Table 2 is available in electronic form at http://www.aanda.org Reference:WR 35a: A new double-lined spectroscopic binary Authors: Gamen, R.; Collado, A.; Barbá, R.; Chené, A.-N.; St-Louis, N. |
Name | Table Head | Description | Unit | UCD |
---|---|---|---|---|
accref | Product key | Access key for the data | N/A | meta.ref.url;meta.dataset |
ssa_location | Location | ICRS location of aperture center | deg | pos.eq |
ssa_dateObs | Date Obs. | Midpoint of exposure | d | time.epoch |
accsize | File size | Size of the data in bytes | byte | N/A |
ssa_dstitle | Title | A compact and descriptive designation of the dataset. | N/A | meta.title;meta.dataset |
ssa_specstart | Band start | Lower value of spectral coordinate | m | em.wl;stat.min |
ssa_specend | Band end | Upper value of spectral coordinate | m | em.wl;stat.max |
ssa_specmid | Mid. Band | Midpoint of region covered in this dataset | m | em.wl;instr.bandpass |
ssa_specext | Bandwidth | Width of the spectrum | m | em.wl;instr.bandwidth |
ssa_targname | Object | Common name of object observed. | N/A | meta.id;src |
ssa_instrument | Instrument | Instrument or code used to produce these datasets | N/A | meta.id;instr |
mime | Type | MIME type of the file served | N/A | meta.code.mime |