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Refining Orbits of Bright Binary Systems
DOI:10.3390/galaxies11010008.png)
摘要
En 中文
We obtained spectra of several bright binary systems (zeta 02 UMa, 2 Lac, and phi Aql), which were mostly observed with photographic plates and whose orbits were not determined very accurately. Each system was monitored for a few years with the 81-cm telescope equipped with an echelle spectrograph at the Three College Observatory in North Carolina. The spectra were taken in a wavelength range between 4000 and 7900 angstrom with a spectral resolution of R similar to 12,000. Radial velocity measurements were done using cross-correlation in selected spectral regions or by measuring positions of individual spectral lines. Refined orbits and stellar parameters are presented.
Keyword:
spectroscopy
binary system
stars
期刊
IF:
3.8
论文数:
829
被引数:
2.1K

