Planning Near-Earth Asteroid Observations on a 1-Meter Class Telescope
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Văduvescu, Ovidiu et al.
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2006
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Pioneer Anomaly? Gravitational Pull due to the Kuiper BeltIn this work, we study the gravitational influence of the material extending from Uranus orbit to the Kuiper belt and beyond on objects moving within these regions. We conclude that a density distribution given by ρ (r)=(1)/(r) (for r >= 20 AU) generates a constant acceleration towards the Sun on those objects, which, with the proper amount of massde Diego, José A. et al.
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Photometry and Spectroscopy of Bright Stars in the Carina dSph GalaxyWe present the results of a spectroscopic analysis of bright stars in the Carina dSph galaxy. We collected low-resolution FORS2@VLT spectra of ≈ 200 stars. Our spectroscopic targets have been selected among the evolved Carina stars, in particular we selected low-mass, old Red Giant, Asymptotic, and Horizontal Branch stars, as well as intermediateMonelli, M. et al.
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Perseus anomalous emission as seen with VSANot AvailableWatson, Robert et al.
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Oxygen in Metal-Rich Stars: Abundances from [O I] 6300, OI 7771 5 and Near-UV OHOxygen abundances of a large number of metal-rich stars, with and without known planets, were derived from the forbidden line [O I] 6300 Å, the OI 7771-5 Å triplet and from near-UV OH lines. Non-LTE corrections were calculated and applied to the LTE abundance results derived from the OI 7771-5 Å triplet. Spectral synthesis was performed for severalEcuvillon, A. et al.
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OO Serpentis, an Intermediate Object between FUors and EXors?OO Serpentis is a deeply embedded young star which brightened by 5 mag in Kband between 1994 and 1995, and gradually faded afterwards. In many respects the star and its outburst is very similar to the well-known young eruptive stars (FUors and EXors). We monitored the eruption of OO Ser for 20 months with the Infrared Space Observatory in the 3.6Kóspál, A. et al.
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02006