@article{setiawan_study_2000,
	title = {A study of the activity of {G} and {K} giants through their precise radial velocity. {Breaking} the 10-m/sec accuracy with {FEROS}.},
	volume = {102},
	issn = {0722-6691},
	url = {https://ui.adsabs.harvard.edu/abs/2000Msngr.102...13S},
	abstract = {Asteroseismology is an indispensable tool that uses the properties of stellar oscillations to probe the internal structure of stars. This can provide a direct test of stellar structure and evolution theory. Precise stellar radial velocity (RV) measurements made in recent years have not only discovered the first extra-solar planets, but have also uncovered new classes of low-amplitude variable stars. One such is represented by the K giant stars which exhibit RV variations with amplitudes in the range of 50-300 m/s (Walker et al. 1989, Hatzes \& Cochran 1993,1994 ab). This variability is multi-periodic and occurring on two time- scales: less than 10 days and several hundreds of days.},
	journal = {The Messenger},
	author = {Setiawan, J. and Pasquini, L. and da Silva, L. and Hatzes, A. and von der Luhe, O. and Kaufer, A. and Girardi, L. and de La, Reza R. and de Medeiros, J. R.},
	month = dec,
	year = {2000},
	pages = {13--17},
}

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