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A.G.G.M. Tielens L.B.F.M. Waters F.J. Molster K. Justtanont 《Astrophysics and Space Science》1997,255(1-2):415-426
This paper reviews spectra obtained with the SWS on board of ISO of dust shells around O-rich objects. These spectra reveal
the presence of many new emission features between 10 and 45 μm. These bands are generally much narrower than the well-known
10 and 20 μm silicates features. The strength of these features relative to the underlying broad continuum varies from source
to source (≅ 5-50%). The 10 μm region shows evidence for the presence of Al2O3 grains. At longer wavelength, the spectra are
dominated by features due to crystalline olivine and pyroxene. The exact peak position of these features shows that the emitting
grains consist of the Mg-rich end-members of these minerals with an Fe-content of < 10%. The underlying continuum is attributed
to amorphous silicate grains.
These observations of aluminum-rich and magnesium-rich compounds compare well with the thermodynamic condensation sequence
of minerals expected for O-rich outflows. The observations also imply that freeze out (ie., kinetics) of this condensation
sequence at different temperatures is an important characteristic of dust formation in these objects. It is suggested that
the absence of Fe-rich silicates is a natural consequence of the low temperature at which gaseous Fe reacts with Mg-rich silicates
in these outflows, resulting in amorphous grains with little characterizing spectral detail.
This revised version was published online in August 2006 with corrections to the Cover Date. 相似文献
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We have calculated the circumstellar extinction curves produced by dust grains which absorb and scatter the stellar radiation in the shells of pre-main-sequence stars. A Monte Carlo method was used to model the radiative transfer in non-spherical shells. The dependence on the particle size distribution and the dust shell parameters has been examined.The application of the theoretical results to explain the extinction and polarization of the Herbig Be star HD 45677 shows that the dust shell is not disk-like and that very small grains are absent in it. 相似文献
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西准噶尔包古图地区地层火山岩锆石LA-ICP-MS U-Pb年代学研究 总被引：24，自引：11，他引：13
包古图地区位于西准噶尔东南部,区内出露地层主要为石炭系太勒古拉组、包古图组和希贝库拉斯组,为一套巨厚的半深海相-大陆坡相火山-火山碎屑沉积建造。这套地层的时代归属和地层层序长期以来一直存在争议。本文报导了包古图地区实测地层剖面,并从太勒古拉组玄武岩和包古图组及希贝库拉斯组凝灰岩中分别选出锆石,进行了LA-ICP-MS U-Pb年代学研究,获得206Pb/238U加权平均年龄分别为357.5±5.4Ma、332.1±3.0Ma和336.3±2.5Ma。由此确定这套地层属于早石炭世的杜内阶到维宪阶,由下到上依次为太勒古拉组、包古图组和希贝库拉斯组。 相似文献
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L. Colangeli Th. Henning J.R. Brucato D. Clément D. Fabian O. Guillois F. Huisken C. Jäger E.K. Jessberger A. Jones G. Ledoux G. Manicó V. Mennella F.J. Molster H. Mutschke V. Pirronello C. Reynaud J. Roser G. Vidali L.B.F.M. Waters 《Astronomy and Astrophysics Review》2003,11(2-3):97-152
Abstract. Silicate grains in space have attracted recently a wide interest of astrophysicists due to the increasing amount and quality
of observational data, especially thanks to the results obtained by the Infrared Space Observatory. The observations have
shown that the presence of silicates is ubiquitous in space and that their properties vary with environmental characteristics.
Silicates, together with carbon, are the principal components of solid matter in space. Since their formation, silicate grains
cross many environments characterised by different physical and chemical conditions which can induce changes to their nature.
Moreover, the transformations experienced in the interplay of silicate grains and the medium where they are dipped, are part
of a series of processes which are the subject of possible changes in the nature of the space environment itself. Then, chemical
and physical changes of silicate grains during their life play a key role in the chemical evolution of the entire Galaxy.
The knowledge of silicate properties related to the conditions where they are found in space is strictly related to the study
in the laboratory of the possible formation and transformation mechanisms they experience. The application of production and
processing methods, capable to reproduce actual space conditions, together with the use of analytical techniques to investigate
the nature of the material samples, form a subject of a complex laboratory experimental approach directed to the understanding
of cosmic matter. The goal of the present paper is to review the experimental methods applied in various laboratories to the
simulation and characterisation of cosmic silicate analogues. The paper describes also laboratory studies of the chemical
reactions undergone and induced by silicate grains. The comparison of available laboratory results with observational data
shows the essential constraints imposed by astronomical observations and, at the same time, indicates the most puzzling problems
that deserve particular attention for the future. The outstanding open problems are reported and discussed. The final purpose
of this paper is to provide an overview of the present stage of knowledge about silicates in space and to provide to the reader
some indication of the future developments in the field.
Received 25 April 2002 / Published online 14 November 2002
Send offprint requests to: L. Colangeli e–mail: colangeli@na.astro.it 相似文献
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The very large brightness decrease of late-type Herbig Ae/Be stars is believed to be caused by obscuring dust clouds orbiting in the outer parts of their circumstellar disks. The distances of the dust clouds to the central stars have been estimated using the wavelength at maximum flux of the excess near-IR radiation, Wien's displacement law, and a formula derived by Rowan-Robinson (1980). The critical masses of these clouds were calculated employing Chandrasekhar's (1943) formula. The minimum size of the dust grains in the obscuring clouds was estimated using Aumannet al.'s (1984) formula they had applied to the star Lyr. However, it can be about ten times smaller if the dust grains are situated at the back of the cloud. The average size of these grains has been determined by assuming a size distribution similar to that in the asteroidal belt (Dohnanyi, 1969) and in the interstellar medium (Mathiset al., 1977). Their number density was determined by means of the extinction power of the dust cloud at theV pass-band. The results of our calculations show that above parameters are similar to those in our solar system. Therefore, we believe that most probably (a) the formation of planetesimals in the circumstellar disks of Herbig Ae/Be stars is on-going; and (b) the obscuring clouds will, in the long run, become planet-like objects.Paper presented at the Conference onPlanetary Systems: Formation, Evolution, and Detection held 7–10 December, 1992 at CalTech, Pasadena, California, U.S.A. 相似文献
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D Parker SE Kerwath TF Næsje CJ Arendse FJ Keulder-Stenevik K Hutchings 《African Journal of Marine Science》2017,39(2):153-166
White stumpnose Rhabdosargus globiceps is the main target of the linefishery in Saldanha Bay. Increased fishing pressure over the last three decades, particularly by the recreational sector, has led to concerns regarding sustainability of the local white stumpnose stock. The fishery was exceptionally productive between 2006 and 2008, with an estimated annual catch of 141.2 tonnes (t). Only 3% of boat outings surveyed were commercial boats targeting white stumpnose, yet this sector accounted for 39.3 t (31%) of the average annual catch. The recreational boat sector accounted for most of the catch (70.0 t), and the recreational shore sector the least (31.9 t). Commercial boat catch per unit effort (CPUE; 3.7 fish angler–1 h–1) was more than 10 times that of recreational boats (0.3 fish angler–1 h–1). White stumpnose catch length-frequency differed significantly (p < 0.01) between the fishing sectors, with the commercial sector retaining larger fish (34.7 cm [SD 5.9]) than the recreational boat (33.9 cm [SD 5.9]) and shore (30.4 cm [SD 5.8]) sectors. A decline in commercial CPUE (2000–2015) of approximately 40% and a concomitant severe decline (>95%) in survey data for juvenile white stumpnose CPUE (2007–2016) indicate that the current rate of exploitation is not sustainable. Recovery of the white stumpnose stock will require a decrease in fishing mortality. Possible management regulations include sector-specific effort limitations, extending the ‘no take’ marine protected area, reducing the recreational-sector bag limit to 5 fish person–1 day–1, implementing a commercial-sector bag limit, and increasing the minimum size limit to 30 cm TL. 相似文献
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