Search Results - "Waters, L.B.F.M."
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The building blocks of planets within the 'terrestrial' region of protoplanetary disks
Published in Nature (25-11-2004)“…Our Solar System was formed from a cloud of gas and dust. Most of the dust mass is contained in amorphous silicates, yet crystalline silicates are abundant…”
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Dust in protoplanetary disks: observations
Published in EPJ Web of conferences (01-01-2015)“…Solid particles, usually referred to as dust, are a crucial component of interstellar matter and of planet forming disks surrounding young stars. Despite the…”
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The role of laboratory experiments in the characterisation of silicon-based cosmic material
Published in The Astronomy and astrophysics review (01-04-2003)“…Silicate grains in space have attracted recently a wide interest of astrophysicists due to the increasing amount and quality of observational data, especially…”
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Laboratory mid-IR spectra of equilibrated and igneous meteorites. Searching for observables of planetesimal debris
Published in Icarus (New York, N.Y. 1962) (01-06-2018)“…•We provide new mid-IR transmission spectra of powdered meteorites.•We can spectroscopically recognise and distinguish between different meteorite types.•We…”
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Comet-like mineralogy of olivine crystals in an extrasolar proto-Kuiper belt
Published in Nature (London) (04-10-2012)“…Analysis of the 69-micrometre spectral band of olivine crystals in the β Pictoris planetary system shows that they can be associated with an extrasolar…”
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Sequential Star Formation in RCW 34: A Spectroscopic Census of the Stellar Content of High-Mass Star-Forming Regions
Published in The Astrophysical journal (20-04-2010)Get full text
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Spectroscopic parameters for silacyclopropynylidene, SiC 2, from extensive astronomical observations toward CW Leo (IRC +10216) with the Herschel satellite
Published in Journal of molecular spectroscopy (2012)“…[Display omitted] ► SiC 2 is an abundant molecule in circumstellar shells of carbon-rich late-type stars. ► Lines have been detected beyond 1 THz in…”
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An update of the Amsterdam Light Scattering Database
Published in Journal of quantitative spectroscopy & radiative transfer (01-07-2006)“…We present an update of the Amsterdam Light Scattering Database located at http://www.astro.uva.nl/scatter. We give a detailed explanation and clarification of…”
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The composition and size distribution of the dust in the coma of Comet Hale–Bopp
Published in Icarus (New York, N.Y. 1962) (01-12-2005)“…We discuss the composition and size distribution of the dust in the coma of Comet Hale–Bopp. We do this using a model fit for the infrared emission measured by…”
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The Compact Circumstellar Material around OH 231.8+4.2
Published in The Astrophysical journal (01-08-2006)“…We have observed the bipolar post-asymptotic giant branch candidate OH 231.8+4.2, using the mid-infrared interferometer MIDI and the infrared camera with the…”
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Binarity as a Key Factor in Protoplanetary Disk Evolution: Spitzer Disk Census of the E Chamaeleontis Cluster
Published in The Astrophysical journal (10-12-2006)“…The formation of planets is directly linked to the evolution of the circumstellar (CS) disk from which they are born. The dissipation timescales of CS disks…”
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Laboratory studies of scattering matrices for randomly oriented particles: potentials, problems, and perspectives
Published in Journal of quantitative spectroscopy & radiative transfer (01-06-2003)“…A number of issues relevant to laboratory studies of scattering matrices as functions of the scattering angle for randomly oriented particles in the visible…”
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Scattering matrices and reflectance spectra of forsterite particles with different size distributions
Published in Journal of quantitative spectroscopy & radiative transfer (01-01-2006)“…We present measurements of the complete scattering matrix as a function of the scattering angle of three different samples of forsterite particles in random…”
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WWW scattering matrix database for small mineral particles at 441.6 and [formula omitted]
Published in Journal of quantitative spectroscopy & radiative transfer (2005)“…We present a new extensive database containing experimental scattering matrix elements as functions of the scattering angle measured at 441.6 and 632.8 nm for…”
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The equatorial disc of the Be star X Persei
Published in Monthly notices of the Royal Astronomical Society (01-06-1998)“…We study the long-term behaviour of the equatorial disc of the Be/X-ray binary X Persei (X Per), combining new low-resolution IUE spectra and IR photometry…”
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SEQUENTIAL STAR FORMATION IN RCW 34: A SPECTROSCOPIC CENSUS OF THE STELLAR CONTENT OF HIGH-MASS STAR-FORMING REGIONS
Published in The Astrophysical journal (20-04-2010)Get full text
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Discovery of extended radio emission in the young cluster Wd1
Published in Monthly notices of the Royal Astronomical Society (01-10-1998)“…We present 10-μm ISO-SWS and Australia Telescope Compact Array observations of the region in the cluster Wd1 in Ara centred on the B[e] star Ara C. An ISO-SWS…”
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Infrared, submillimeter, and millimeter observations of the Soft Gamma-Ray Repeaters
Published in Advances in space research (01-01-1998)“…The Soft Gamma-Ray Repeaters appear to be a completely new manifestation of neutron stars. SGR 1806-20 and SGR 1900+14 may have highly unusual stellar…”
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Comet Hale-Bopp, Circumstellar Dust, and the Interstellar Medium
Published in Earth, moon, and planets (01-09-1997)“…The infrared spectrum of comet Hale-Bopp, as observed with the Infrared Space Observatory (ISO), presents astonishing similarities with those of the dusty…”
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