Spectrum of LSR J0745+2627 obtained using XShooter at VLT, Paranal Observatory. No smoothing has been applied to this spectrum. (1 data file).
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..
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Spectrum of LSR J0745+2627 (Catalan+, 2012)Zhang, Z. H. et al.92012
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Spicule emission profiles observed in He i 10 830 Å
Aims:Off-the-limb observations with high spatial and spectral resolution will help us understand the physical properties of spicules in the solar chromosphere. Methods: Spectropolarimetric observations of spicules in the He i 10 830 Å multiplet were obtained with the Tenerife Infrared Polarimeter on the German Vacuum Tower Telescope at the
Sánchez-Andrade Nuño, B. et al.Advertised on:
92007 -
Spitzer IRS Spectroscopy of High-Mass Precursors of Planetary Nebulae
We present Spitzer IRS observations of a small sample of heavily obscured IRAS sources displaying both the infrared and OH maser emission characteristic of OH/IR stars on the asymptotic giant branch (AGB), but also radio continuum emission typical of ionized planetary nebulae (PNe), the so-called OHPNe. Our observations show that their mid-infrared
García-Hernández, D. A. et al.Advertised on:
92007 -
Spitzer Space Telescope studies of primitive solar system objects
Not Available
Emery, J. P.Advertised on:
92008 -
Stability and formation of the resonant system HD 73526
Context: Based on radial velocity measurements, it has been found that the two giant planets detected around the star HD 73526 are in 2:1 resonance. However, as our numerical integration shows, the derived orbital data for this system result in chaotic behavior of the giant planets, which is uncommon among the resonant extrasolar planetary systems
Sándor, Zs. et al.Advertised on:
92007 -
Standing on the shoulder of a giant: ISAAC, Antu, and star formation
In this article, we hope to illustrate the great qualitative and quantitative strides that star-formation studies have taken in the past few years, by looking at three highlights from our own work using the ESO Very Large Telescope UT1, Antu, and its facility near-infrared camera/spectrograph, ISAAC. In particular, we have chosen examples which
McCaughrean, M. et al.Advertised on:
92002