Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S298(9), p. 429-429, 2013
DOI: 10.1017/s1743921313006959
Full text: Unavailable
AbstractWe are carrying out near-infrared spectroscopy of Cepheids in the Galactic nuclear disk. The H-band spectra taken with SUBARU/IRCS indicate that their kinematics are consistent with the rotation of the nuclear disk.