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
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...
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...