Spectroscopy of Pluto at six longitudes, 380-930 nm
We have obtained spectra of the Pluto-Charon pair (unresolved) in the wavelength range 380-930 nm with resolution ~450 at six roughly equally spaced longitudes...
Spectroscopy of Post-AGB A-Supergiant HD 101584 (IRAS 11385-5517)
In the high resolution optical spectra we identified forbidden lines of [OI] and [CI], which indicate the presence of low excitation nebula. There are many...
Spectroscopy of Post-AGB Candidate HD 331319 (IRAS 19475+3119)
HD 331319 is a F3 Ib star with a detached cold circumstellar dust shell with far-IR colours similar to planetary nebulae. From an analysis of high resolution...
Spectroscopy of Post-AGB Candidate IRAS 10215-5916
IRAS 10215-5916 was classified as a post-AGB star and also as a massive red supergiant. It was also found to be a spectroscopic binary. In our high resolution...
We have carried out an analysis of the high resolution optical spectra of post-AGB candidates SAO 85766 (IRAS 18062+2410), SAO 34504 (IRAS 22272+5435), HD...
Spectroscopy of Resolved Stellar Populations in Dwarf Galaxies with the European Extremely Large Telescope
Samples of line-of-sight velocities and metallicities for hundreds individual red giant branch stars in Milky Way satellite galaxies have been obtained in the...
Spectroscopy of the Earth Observed as a Distant Planet
Through ground-based observations of the Earth's spectrum from California, satellite observations of clouds, and an atmospheric radiative transfer code, we have...
Spectroscopy Of The Earth Observed As A Distant Planet
Since the discovery of the first planet outside the solar system, the number of planet detections is increasing exponentially. Although we have not been capable...