The effects of ellipticity and substructure on estimates of cluster density profiles based on lensing and kinematics     

Massimo Meneghetti  Matthias Bartelmann  Adrian Jenkins  Carlos Frenk 《Monthly notices of the Royal Astronomical Society》2007,381(1):171-186

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cD galaxy contribution to the strong lensing cross-sections of galaxy clusters     

Massimo Meneghetti  Matthias Bartelmann  Lauro Moscardini 《Monthly notices of the Royal Astronomical Society》2003,346(1):67-77

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Authenticating the recovery location of meteorites: The case of Castenaso     

Luigi Folco  Massimo D'Orazio  Natale Perchiazzi 《Meteoritics & planetary science》2007,42(3):321-330

Abstract— This forensic work aims to authenticate the recovery location of Castenaso, a 120 g ordinary chondritic (L5) meteorite reportedly found in 2003 along the sandy bank of the Idice Stream, near the village of Castenaso (Bologna, Emilia‐Romagna, Italy). Using the hypothesis that Castenaso was instead a hot‐desert meteorite, we conducted a comparative mineralogical and geochemical study of major weathering effects on European and Saharan ordinary chondrites as potential markers of the environment where Castenaso resided during its terrestrial lifetime. Inductively coupled plasma‐mass spectrometry (ICP‐MS) data reveals that Castenaso is significantly enriched in Sr, Ba, Tl, and U, and suggests geochemical alteration in a hot‐desert environment. The alteration is minor: Castenaso is not coated by desert varnish and does not show significant light rare earth element (LREE) enrichment or loss of Ni and Co. The apparent contrast in size, morphology, and composition between the soil particles filling the external fractures of Castenaso and those from the bank of the Idice Stream observed under the scanning electron microscope (SEM) suggests that Castenaso did not reside at the reported find location. Abraded quartz grains (up to 1 mm in size) in Castenaso are undoubtedly from a hot‐desert eolian environment: they are well‐rounded and show external surfaces characterized by the presence of dish‐shaped concavities and upturned silica plates that have been subject to solution‐precipitation and subsequent smoothing. We therefore conclude that Castenaso is one of the many hot‐desert ordinary chondrite finds, probably from the Sahara, that is currently available on the market. This forensic work provides the scientific grounds for changing the name of this meteorite.  相似文献   

A refined genetic model for the Laisvall and Vassbo Mississippi Valley-type sandstone-hosted deposits,Sweden: constraints from paragenetic studies,organic geochemistry,and S,C, N,and Sr isotope data     

Nicolas J. Saintilan  Jorge E. Spangenberg  Elias Samankassou  Kalin Kouzmanov  Massimo Chiaradia  Michael B. Stephens  Lluís Fontboté 《Mineralium Deposita》2016,51(5):639-664

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High crustal diversity preserved in the lunar meteorite Mount DeWitt 12007 (Victoria Land,Antarctica)          下载免费PDF全文

Alberto Collareta  Massimo D'Orazio  Maurizio Gemelli  Andreas Pack  Luigi Folco 《Meteoritics & planetary science》2016,51(2):351-371

The meteorite Mount DeWitt (DEW) 12007 is a polymict regolith breccia mainly consisting of glassy impact‐melt breccia particles, gabbroic clasts, feldspathic clasts, impact and volcanic glass beads, basaltic clasts, and mingled breccia clasts embedded in a matrix dominated by fine‐grained crystals; vesicular glassy veins and rare agglutinates are also present. Main minerals are plagioclase (typically An_>85) and clinopyroxene (pigeonites and augites, sometimes interspersed). The presence of tranquillityite, coupled with the petrophysical data, the O‐isotope data (Δ¹⁷O = ?0.075), and the FeO_tot/MnO ratios in olivine (91), pyroxene (65), and bulk rock (77) indicate a lunar origin for DEW 12007. Impactites consist of Al‐rich impact‐melt splashes and plagioclase‐rich meta‐melt clasts. The volcanic products belong to the very low titanium (VLT) or low titanium (LT) suites; an unusual subophitic fragment could be cryptomare‐related. Gabbroic clasts could represent part of a shallow intrusion within a volcanic complex with prevailing VLT affinity. DEW 12007 has a mingled bulk composition with relatively high incompatible element abundances and shows a high crustal diversity comprising clasts from the Moon's major terranes and rare lithologies. First‐order petrographic and chemical features suggest that DEW 12007 could be launch‐paired with other meteorites including Y 793274/981031, QUE 94281, EET 87521/96008, and NWA 4884.  相似文献   

‘Isolated base-of-slope aprons’: An oxymoron for shallow-marine fan-shaped,temperate-water,carbonate bodies along the south-east Salento escarpment (Pleistocene,Apulia, southern Italy)     

Marcello Tropeano  Luigi Spalluto  Demetrio Meloni  Massimo Moretti  Luisa Sabato 《Sedimentology》2022,69(1):345-371

This paper regards the lower Pleistocene temperate-water carbonate deposits disconformably overlying an escarpment made up of faulted Cretaceous to Miocene limestones of the Apulia Foreland (southern Italy). Study deposits discontinuously crop out along the present-day eastern Salento sea cliff, and form isolated fan-shaped bodies, up to 1 km wide and up to 40 to 50 m thick, each of them covering an area of a few square kilometres. The internal arrangement of beds is represented by up to 25° to 30° lobate, seaward dipping clinobeds thinning and onlapping onto a rocky foreslope in the proximal sector and passing to gently inclined to sub-horizontal strata in the distal sector. Seven facies were distinguished, mainly composed of coarse-grained skeletal carbonates made up of a heterozoan association including coralline algae, large and small benthic foraminifera, echinoids, molluscs, bryozoans and serpulids. Since clinobeds were formed thanks to hyperconcentrated density flows (grain flows) bypassing the upper part of the inherited escarpment, these skeletal grains represent ex situ deposits whose shallow-marine factory was located upward (landward) with respect to the bypassed zone, likely in the almost flat area on top of the Salento Peninsula. Clinobeds are often affected by tens of metres wide and long channel-like structures interpreted as landslide scars. Inside these gullies, contorted beds (slumps) or matrix-supported intra-bioclastic floatstone/rudstone (massive deposits) are present. The occurrence of supercritical-flow structures (for example, backset-bedded beds) indicates the development of hydraulic jumps along the steep slope of gullies. Since these clinostratified, fan-shaped carbonate bodies represent carbonate slopes, and that the latter are known as aprons, normally related to linear sourced sediments, an acceptable oxymoron for studied fan-shaped carbonate bodies is suggested: ‘isolated base-of-slope aprons’.  相似文献   

Geochronological study of zircons from continental crust rocks in the Frido Unit (southern Apennines)     

Salvatore Laurita  Giacomo Prosser  Giovanna Rizzo  Antonio Langone  Massimo Tiepolo  Alessandro Laurita 《International Journal of Earth Sciences》2015,104(1):179-203

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Structure of the vertical velocity field analyzed with a Doppler Sodar     

Angelo Ricotta  Massimo Berico  Salvatore Mazzola 《Boundary-Layer Meteorology》1983,27(4):311-325

Fifteen hours of Sodar echoes, collected during the 4th Environmental CEC Campaign at Turbigo, Italy, in September 1979, have been analyzed. We discuss the vertical profiles and the time evolution of the second and third statistical moments of the vertical component of wind velocity, measured at a rate of one height-profile every 6 s for a height range of 1000 m and a vertical resolution of 29 m. We also analyze the power spectra of the vertical velocity.  相似文献   

Long-term radial velocity variations in some Be stars     

Elio Antonello  Massimo Fracassini  Laura Enrica Pasinetti  Livio Pastori 《Astrophysics and Space Science》1982,83(1-2):381-390

All the radial velocities (RV) available in the literature since the beginning of the century for the Be stars EW Lac, 28 Tau, Tau, KX And, KY And, CX Dra and 88 Her, are assembled. When possible, a periodogram analysis has been performed to search for eventual periodic phenomena.The following conclusions have been drawn: EW Lac could be a spectroscopic binary with a period of about 40 years; 28 Tau shows some indications of regular long-term RV variations on the time scale of decades; a probable recurrent shell activity of Tau could be hypothesized. Some useful indications for KX and KY And are given, whereas it is not possible to draw any conclusion for CX Dra and 88 Her owing to the lack of data.  相似文献   

Spectrographic observations of omicron andromedae from 1967 to 1976     

Massimo Fracassini  Laura E. Pasinetti  Livio Pastori 《Astrophysics and Space Science》1977,49(1):145-167

The results of qualitative analysis and radial velocity (RV) determinations from 1967 to 1976 are given. These analyses show sometimes the presence of a thin variable shell also in the years 1967–1974, before the appearance of the envelope. Intensity variations of the metallic lines seem to indicate that in the same period changes of temperature and/or electron pressure may occur in the photospheric layers. In the period 1975–76, the considerable range ofRV and the variability of the shell features show that the shell is rather active. Some conspicuousRV variations seem to be correlated to brightness changes. TheRV do not confirm the periods suggested by the photometric observations. A periodogram analysis givesRV curves with a poor evidence of periodicity. However, the periodP=1^d.5845 obtained from this analysis, close to that of Schmidt, seems to confirm Schmidt's hypothesis of a contact binary system. The periodogram analysis of theRV during the years 1900–1976 and some physical arguments, suggest a probable photospheric activity or an invisible companion with the observed shell period of 30 yr. The duplicity, suggested by Kí and Harmanec (1975) for all the Be stars, could be yet questioned foro And.Thesis for the degree of Applied Physics.  相似文献